cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: Invisible Abuse: Utah's Response to Emotional Child Abuse
Creators: name: Sirrine, Janae
Publisher: name: Utah State University
Year: 2010

description: The very nature of emotional child abuse makes it difficult to detect and report. Nevertheless, scholars and professionals in the field of child welfare have identified emotional abuse as being equally detrimental to children as physical abuse and neglect. Many states, including Utah, have unclear definitions of emotional child abuse. The purpose of this study is to interpret how Utah has used its statute on emotional abuse in the court system and whether the current definition of emotional child abuse has given Utah’s courts enough information and direction to prosecute those who emotionally abuse children. Data was collected by researching the legislative history of the statute, compiling cases of emotional abuse that have come before the Utah Court of Appeals, and interviewing professionals who have dealt with cases of emotional abuse in Utah. This study concludes that although child emotional maltreatment, once reported, is being adequately treated therapeutically when cases involve other types of abuse, it is not being addressed adequately in the court system when emotional abuse is solely in question. There is a need for more direction in the legal community in defining and responding to emotional child abuse.
title: To What Extent Do Local Farmers' Markets, Community Supported Agriculture Programs, and Community Gardens Help Low-Income Families Improve Access to Fresh, Local Produce?
Creators: name: Somsen, Christy Gene
Publisher: name: Utah State University
Year: 2010

description: Farmers’ Markets, Community Supported Agriculture (CSA) Programs, and Community Gardens have been developed to help farmers. Many times, they also aim to help low-income families improve access to fresh produce. Often, these programs may end up helping a larger amount of middle class families instead of lower class families. There have been many programs developed to try to better help low-income families such as the Women Infant and Children (WIC) Farmers’ Market Nutrition Program (FMNP) and allowing farmers to accept WIC Cash Value Vouchers (CVV), which allows WIC participants to buy fresh produce. Farm to School Programs have also been great programs for helping farmers and improving fruit and vegetable intake in students. Many states have implemented these programs and have given great examples of how these programs can be developed and put into action. Utah has farmers’ markets, a few CSAs, and some community gardens that all could be improved upon. Utah does not employ the WIC FMNP nor allow farmers to accept the WIC CVVS. There are also only a few Farm to School Programs in Utah. These are some great programs that could be implemented in Utah to better help the local farmers and community.
title: Genetic and Biochemical Studies of Plasmid pIR52-1 in Lactobacillus helveticus
Creators: name: Tramp, Cody Alexander
Publisher: name: Utah State University
Year: 2010

description: Lactobacillus helveticus is a species of lactic acid bacteria. These bacteria, which produce lactic acid as a major product of carbohydrate metabolism, are used industrially to produce cheese and other fermented dairy products (Ebringer et al., 2008). Many species of lactic acid bacteria also possess probiotic characteristics and when ingested potentially confer increased immune function, regulate gut microbiota, and improve digestion in the host (Reid, 2008). Genetic studies of these probiotic effects and other characteristics of L. helveticus and related species have been hindered by the lack of stably replicating plasmid vectors. Plasmid vectors for several Lactobacillus species have been constructed, but these are often derived from broad host range plasmids and may not be stably maintained over many generations (Fang et al., 2008; Thompson et al., 2001). In L. helveticus specifically, a small number of attempts have been made at adapting plasmid vectors for use in genetic studies, but as the source plasmids were not native to L. helveticus, they were either unable to replicate extrachromosomally or be maintained over many generations (Hagen et al., 2010; Thompson et al., 2001).
title: The Temple Recommend: A Solution to the Free-Rider Problem
Creators: name: Bowles, Austin
Publisher: name: Utah State University
Year: 2010

description: ﻿Temple worship and geographical boundaries are unique features of the Church of Jesus Christ of Latter-day Saints (LDS Church). Our research uses economic theory to understand how the organizational benefits of the temple recommend system and the geographical ward boundaries may solve the market failures associated with religious organizations. These features of the LDS Church will be used to create a framework for understanding how the church limits free-riding and sub-optimal participation, which would result in increased efficiency and production of large religious benefits. Because the market failures faced by the church are the same as those faced by other religious groups and similar to those faced by clubs, this research provides insights into possible solutions for groups besides the LDS church.
The enigmatic pair of dwarf galaxies Leo IV and Leo V: coincidence or common origin?
Creators: name: de Jong, Jelte T. A.
name: Martin, Nicolas F.
name: Rix, Hans-Walter
name: Smith, Kester W.
name: Jin, Shoko
name: Maccio', Andrea V.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We have obtained deep photometry in two 1x1 degree fields covering the close pair of dwarf spheroidal galaxies (dSph) Leo IV and Leo V and part of the area in between. We find that both systems are significantly larger than indicated by previous measurements based on shallower data and also significantly elongated. With half-light radii of r_h=4'.6 +- 0'.8 (206 +- 36 pc) and r_h=2'.6 +- 0'.6 (133 +- 31 pc), respectively, they are now well within the physical size bracket of typical Milky Way dSph satellites. Their ellipticities of epsilon ~0.5 are shared by many faint (M_V>-8) Milky Way dSphs. The large spatial extent of our survey allows us to search for extra-tidal features with unprecedented sensitivity. The spatial distribution of candidate red giant branch and horizontal branch stars is found to be non-uniform at the ~3 sigma level. This substructure is aligned along the direction connecting the two systems, indicative of a possible `bridge' of extra-tidal material. Fitting the stellar distribution with a linear Gaussian model yields a significance of 4 sigma for this overdensity, a most likely FWHM of ~16 arcmin and a central surface brightness of ~32 mag arcsec^{-2}. We investigate different scenarios to explain the close proximity of Leo IV and Leo V and the possible tidal bridge between them. Orbit calculations demonstrate that they are unlikely to be remnants of a single disrupted progenitor, while a comparison with cosmological simulations shows that a chance collision between unrelated subhalos is negligibly small. Leo IV and Leo V could, however, be a bound `tumbling pair' if their combined mass exceeds 8 +- 4 x 10^9 M_sun. The scenario of an internally interacting pair appears to be the most viable explanation for this close celestial companionship. (abridged)
description: 9 pages, 8 figures, small number of minor textual changes, accepted for publication in Astrophysical Journal
Two-Phase Galaxy Formation
Creators: name: Cook, M.
name: Lapi, A.
name: Granato, G. L.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We propose and test a scenario for the assembly and evolution of luminous matter in galaxies which substantially differs from that adopted by other semianalytic models. As for the dark matter (DM), we follow the detailed evolution of halos within the canonical LCDM cosmology using standard Montecarlo methods. However, when overlaying prescriptions for baryon evolution, we take into account an effect pointed out in the past few years by a number of studies mostly based on intensive N-body simulations, namely that typical halo growth occurs in two phases: an early, fast collapse phase featuring several major merger events, followed by a late, quiescent accretion onto the halo outskirts. We propose that the two modes of halo growth drive two distinct modes for the evolution of baryonic matter, favoring the development of the spheroidal and disc components of galaxies, respectively. We test this idea using the semianalytic technique. Our galaxy formation model envisages an early coevolution of spheroids and the central supermassive black holes, already tested in our previous works, followed by a relatively quiescent growth of discs around the preformed spheroids. In this exploratory study, we couple our model to the spectrophotometric code GRASIL, and compare our results on several properties of the local galaxy population with observations, Finding an encouraging agreement.
description: 16 pages, 21 figures, MNRAS Accepted 23/04/2009
Effects of Mutual Transits by Extrasolar Planet-Companion Systems on Light Curves
Creators: name: Sato, Masanao
name: Asada, Hideki
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: We consider the effects of mutual transits by extrasolar planet-companion systems (in a true binary or a planet-satellite system) on light curves. We show that induced changes in light curves depend strongly on a ratio between a planet-companion's orbital velocity around their host star and a planet-companion's spin speed around their common center of mass. In both the slow and fast spin cases (corresponding to long and short distances between them, respectively), a certain asymmetry appears in light curves. We show that, especially in the case of short distances, occultation of one faint object by the other, while the transit of the planet-companion system occurs in front of its parent star, causes an apparent increase in light curves and characteristic fluctuations appear as important evidence of mutual transits. We show also that extrasolar mutual transits provide a complementary method of measuring the radii of two transiting objects, their separation and mass, and consequently identifying them as a true binary, planet-satellite system or others. Monitoring $10^5$ stars for three years with Kepler may lead to a discovery of a second Earth-Moon-like system if the fraction of such systems for an averaged star is larger than 0.05, or it may put upper limits on the fraction as f < 0.05.
description: 15 pages, 6 figures, 1 table; text improved, typos corrected; PASJ in press
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ð¹ ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: Ð ÑÐ´Ð°ÐºÐ¾Ð²Ð°, ÐÐ»ÑÐ³Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÐµÐºÐ»Ð°Ð¼Ð½Ð°Ñ ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ñ
Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸
ÑÐµÐºÐ»Ð°Ð¼Ð½Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
ÑÐµÐºÐ»Ð°Ð¼Ð½ÑÐ¹ Ð±ÑÐ´Ð¶ÐµÑ

description: Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ð¹ ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ð¸ ÐÐÐ Â«ÐÐ¸Ð¾Ð»ÐµÑ ÐÑÐ¸Ð¼Â» Ð´Ð»Ñ ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¸Ð±ÑÐ»Ð¸. ÐÑÐ» Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ SWOT-Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ ÑÐ¸Ð»ÑÐ½ÑÐµ Ð¸ ÑÐ»Ð°Ð±ÑÐµ ÑÑÐ¾ÑÐ¾Ð½Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÑÐ½Ð¾ÑÐ½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð±ÑÐ»Ð¸ Ð²ÑÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÑ Ð¼Ð°ÑÑÐ°Ð¶Ð½ÑÑ ÑÐ°Ð»Ð¾Ð½Ð¾Ð² Â«Ð¢Ð°Ð¹ ÐÑÐ¸Ð¼Â». Ð¢Ð°ÐºÐ¶Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð»ÑÑ ÑÐµÐºÐ»Ð°Ð¼Ð½ÑÐ¹ Ð±ÑÐ´Ð¶ÐµÑ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ñ ÑÐµÐ»ÑÑ Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð·Ð°ÑÑÐ°ÑÐµÐ½Ð½ÑÑ ÑÐµÑÑÑÑÐ¾Ð². ÐÑÐ»Ð¸ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð½ÐµÐ´Ð¾ÑÑÐ°ÑÐºÐ¸ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸, ÑÐ°ÐºÐ¸Ðµ ÐºÐ°Ðº Ð¾ÑÑÑÑÑÑÐ²Ð¸Ðµ ÑÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ð³Ð¾ Ð¾ÑÐ´ÐµÐ»Ð°, ÑÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ð¹ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ Ð¸ Ð¿ÑÐ¸Ð½ÑÑÑ Ð¼ÐµÑÑ Ð² ÑÑÑÑÐ°Ð½ÐµÐ½Ð¸Ð¸ ÑÑÐ¸Ñ Ð½ÐµÐ´Ð¾ÑÑÐ°ÑÐºÐ¾Ð². Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð±ÑÐ»Ð° ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð° ÑÐµÐºÐ»Ð°Ð¼Ð½Ð°Ñ ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ñ Ð´Ð»Ñ ÐÐÐ Â«ÐÐ¸Ð¾Ð»ÐµÑ ÐÑÐ¸Ð¼Â». Ð ÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½Ð¾Ð¹ ÑÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ð¹ ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÑ Ðº ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐ¾Ð¹ Ð¿ÑÐ¸Ð±ÑÐ»Ð¸ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸.
Observation of tunable Popescu-Rohrlich correlations through post-selection of a gaussian state
Creators: name: Tasca, D. S.
name: Walborn, S. P.
name: Toscano, F.
name: Ribeiro, P. H. Souto
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We show that non-local Popescu-Rohrlich correlations can be observed in the post-selected results of binned position measurements on a two-party gaussian state. Our experiment is based on the spatial correlations of entangled photons and lens systems. We obtain a maximum violation of the CHSH inequality of 3.42, which corresponds to the implementation of a non-local AND gate with success probability of 0.93. These results do not conflict with quantum mechanics due to the post-selection required, and open up the possibility of experimental investigation of fundamental aspects of Popescu-Rohrlich non-locality with a reliable and simple experimental setup.
description: 4 pages, 3 figures
title: ÐÐµÑÐ¾Ð´Ñ ÑÑÐµÑÐ° Ð·Ð°ÑÑÐ°Ñ Ð¸ ÐºÐ°Ð»ÑÐºÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÐ±ÐµÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸ (ÑÐ°Ð±Ð¾Ñ, ÑÑÐ»ÑÐ³) Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐºÐ¸ÑÐ½Ð¾Ð²Ð°, ÐÐ½Ð°ÑÑÐ°ÑÐ¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð·Ð°ÑÑÐ°ÑÑ
ÑÐ°ÑÑ Ð¾Ð´Ñ
Ð¼ÐµÑÐ¾Ð´Ñ ÑÑÐµÑÐ° Ð·Ð°ÑÑÐ°Ñ
ÐºÐ°Ð»ÑÐºÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸ÑÐµ ÑÐµÐ±ÐµÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸ (ÑÐ°Ð±Ð¾Ñ, ÑÑÐ»ÑÐ³)
ÑÐ½Ð¸Ð¶ÐµÐ½Ð¸Ðµ Ð·Ð°ÑÑÐ°Ñ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐ Â«ÐÐÐ ÐÐ±ÑÑÐ¾Ð²ÑÐºÐ¸Ð¹ Ð·Ð°Ð²Ð¾Ð´Â». Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¿Ð¾Ð´ÑÐ¾Ð±Ð½Ð¾Ðµ Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ Ð·Ð°ÑÑÐ°Ñ ÐºÐ°Ðº Ð¾ÑÐ½Ð¾Ð²Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐµÐºÑÐ° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÑÐµÑÐ° Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼ÐµÑ Ð¿Ð¾ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸. Ð Ð¿ÑÐ¾ÑÐµÑÑÐµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ Ð¿Ð¾Ð´ÑÐ¾Ð´Ñ Ðº ÑÐ¾Ð»ÐºÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾Ð½ÑÑÐ¸Ð¹ Â«Ð·Ð°ÑÑÐ°ÑÑÂ», Â«ÑÐ°ÑÑÐ¾Ð´ÑÂ» Ð¸ Â«Ð¸Ð·Ð´ÐµÑÐ¶ÐºÐ¸Â», Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð¸Ñ ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½Ð°Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ°. Ð¢Ð°Ðº Ð¶Ðµ Ð±ÑÐ»Ð¾ Ð¸Ð·ÑÑÐµÐ½Ð¾ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð¾-Ð¿ÑÐ°Ð²Ð¾Ð²Ð¾Ðµ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð·Ð°ÑÑÐ°Ñ Ð² Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ ÑÑÐµÑÐ° Ð·Ð°ÑÑÐ°Ñ Ð¸ ÐºÐ°Ð»ÑÐºÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÐ±ÐµÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸ Ð² Ð Ð¾ÑÑÐ¸Ð¸ Ð¸ Ð·Ð° ÑÑÐ±ÐµÐ¶Ð¾Ð¼. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð¸ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ¸ Ð·Ð°ÑÑÐ°Ñ Ð½Ð° ÐÐ Â«ÐÐÐ ÐÐ±ÑÑÐ¾Ð²ÑÐºÐ¸Ð¹ Ð·Ð°Ð²Ð¾Ð´Â» Ð±ÑÐ»Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¼ÐµÑÑ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÑÐ³Ð°Ð»ÑÐµÑÐ¸Ð¸ Ð² Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð¸ Ð¿ÑÑÐ¸ ÑÐ½Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð·Ð°ÑÑÐ°Ñ. Ð ÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÑ Ð¼ÐµÑ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÑ Ðº Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐ¾Ð¹ Ð¿ÑÐ¸Ð±ÑÐ»Ð¸ Ð¸ ÑÐ¼ÐµÐ½ÑÑÐµÐ½Ð¸Ñ Ð·Ð°ÑÑÐ°Ñ.
Modelling the final state from binary black-hole coalescences
Creators: name: Rezzolla, Luciano
Publisher: name: arXiv
Year: 2008
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Over the last few years enormous progress has been made in the numerical description of the inspiral and merger of binary black holes. A particular effort has gone into the modelling of the physical properties of the final black hole, namely its spin and recoil velocity, as these quantities have direct impact in astrophysics, cosmology and, of course, general relativity. As numerical-relativity calculations still remain computationally very expensive and cannot be used to investigate the complete space of possible parameters, semi-analytic approaches have been developed and shown to reproduce with very high precision the numerical results. I here collect and review these efforts, pointing out the relative strengths and weaknesses, and discuss which directions are more promising to further improve them.
description: Submitted to CQG, LISA-7 Special Issue
Methylene Blue in Sepsis and Septic Shock – A Systematic Review and Meta-Analysis
Creators: name: Soliman, Karim
name: Oommen, Thomas
name: Dr. Neill KJ Adhikari
name: Kanji, Salmaan
name: Rochwerg, Bram
name: Tran, Alexandre
name: Fox-Robichaud, Alison
name: Seely, Andrew
name: Wax, Randy
name: Cook, Deborah
name: Flynn, Barbara
name: Fernando, Shannon
name: Francois Lamontagne
Publisher: name: OSF Registries
Year: 2024
Subjects: subject: Medicine and Health Sciences
subject: Medical Specialties
subject: Critical Care

description: Systematic review and meta-analysis aimed to understand the potential benefits and harms associated with administration of methylene blue in patients with sepsis and septic shock.
A Search for Asteroids, Moons, and Rings Orbiting White Dwarfs
Creators: name: Di Stefano, Rosanne
name: Howell, Steve B.
name: Kawaler, Steven D.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Do white dwarfs host asteroid systems? Although several lines of argument suggest that white dwarfs may be orbited by large populations of asteroids, transits would provide the most direct evidence. We demonstrate that the Kepler mission has the capability to detect transits of white dwarfs by asteroids. Because white-dwarf asteroid systems, if they exist, are likely to contain many asteroids orbiting in a spatially extended distribution, discoveries of asteroid transits can be made by monitoring only a small number of white dwarfs, compatible with Kepler's primary mission, which is to monitor stars with potentially habitable planets. Possible future missions that survey ten times as many stars with similar sensitivity and minute-cadence monitoring can establish the characteristics of asteroid systems around white dwarfs, such as the distribution of asteroid sizes and semimajor axes. Transits by planets would be more dramatic, but the probability that they will occur is lower. Ensembles of planetary moons and/or the presence of rings around planets can also produce transits detectable by Kepler. The presence of moons and rings can significantly increase the probability that Kepler will discover planets orbiting white dwarfs, even while monitoring only a small number of them.
description: 12 pages, 1 figure; submitted to ApJ, 11 February 2009
Assessing processing speed impairments in radiologically isolated syndrome and multiple sclerosis with advanced brain MRI measures of myelin
Creators: name: Kalau, Olivia
Publisher: name: University of British Columbia
Year: 2024

description: Multiple sclerosis (MS) is a demyelinating disease of the central nervous system that results in characteristic discrete lesions visible on conventional magnetic resonance imaging (MRI), and diffuse damage to the surrounding normal appearing white matter (NAWM). Clinically, MS presents with a wide range of symptoms which often include cognitive impairment (CI), of which processing speed is commonly implicated. Improving our understanding of the biological basis of MS-related CI and future cognitive performance may help to uncover relevant biomarkers and provide opportunities to target these symptoms at earlier stages. People with radiologically isolated syndrome (RIS) can convert to MS and can present with CI patterns similar to MS. Thus, RIS represents a unique opportunity to explore the evolution of CI and associations with early disease biomarkers. Myelin water imaging (MWI) is a histologically validated advanced MRI technique capable of measuring myelin content. From MWI scans, the mean myelin water fraction (MWF) and standard deviation (SD) within a region of interest can be extracted, and the myelin heterogeneity index (MHI) can be calculated (MHI = SD/mean MWF). Here, we used MWI as a biomarker to explore myelin differences in NAWM of people with RIS compared to neurologically healthy controls and investigate the relationship between MWI metrics and processing speed. We detected NAWM myelin damage in RIS, particularly in the corpus callosum, and found that increased NAWM myelin damage, particularly in the cingulum, was associated with slower processing speed in RIS. Additionally, we used MWI to explore longitudinal changes in processing speed in people with MS. In people with progressive MS, lower baseline NAWM MHI, indicative of less myelin damage, was associated with a greater decline in processing speed over time. Overall, these results demonstrate the utility of MWI as a biomarker of myelin specific pathology relevant to clinical symptoms and highlights the complexity of MS-related CI across the spectrum of MS.
title: ÐÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ ÐºÐ°Ðº ÑÐ¿Ð¾ÑÐ¾Ð± ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð¼Ð¸Ð´Ð¶Ð° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«Ð¡ÐµÐ·Ð°ÑÑÑ-ÑÐºÐ¾Â»)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°Ð½ÐµÐ²Ð°, ÐÐ½Ð°ÑÑÐ°ÑÐ¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: ÑÐµÐºÐ»Ð°Ð¼Ð°
ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¸Ð¼Ð¸Ð´Ð¶Ð° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð²Ð¾Ð´Ð° Ð´Ð»Ñ Ð¼ÐµÐ´Ð¸Ð° ÑÐµÑÑÑÑÐ° ÐÐÐ Â«ÐÐ¾Ð¼ÑÐ¾Ð¼Ð¾Ð»ÑÑÐºÐ°Ñ Ð¿ÑÐ°Ð²Ð´Ð°Â» ÐÐ°Ð»ÑÐ³Ð°. Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð²Ð¾Ð´Ð° Ð² Ð¼ÐµÐ´Ð¸Ð° ÑÑÐµÑÐµ. ÐÐ²ÑÐ¾ÑÐ¾Ð¼ Ð±ÑÐ»Ð° ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° PR-Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÐÐÐ Â«ÐÐ¾Ð¼ÑÐ¾Ð¼Ð¾Ð»ÑÑÐºÐ°Ñ Ð¿ÑÐ°Ð²Ð´Ð°Â» ÐÐ°Ð»ÑÐ³Ð°, Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¿Ð¾Ð²Ð¾Ð´Ñ ÑÐ¾Ð·Ð´Ð°Ð²Ð°ÐµÐ¼ÑÐµ Ð´Ð°Ð½Ð½ÑÐ¼ Ð¼ÐµÐ´Ð¸Ð° ÑÐµÑÑÑÑÐ¾Ð¼, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ ÑÑÐ´ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ PR-Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐÐÐ Â«ÐÐ¾Ð¼ÑÐ¾Ð¼Ð¾Ð»ÑÑÐºÐ°Ñ Ð¿ÑÐ°Ð²Ð´Ð°Â» ÐÐ°Ð»ÑÐ³Ð°.
Evidence for a magnetic neutron star in high mass X-ray binary 4U 2206+54 with INTEGRAL/IBIS observations
Creators: name: Wang, W.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The hard X-ray source 4U 2206+54 is a peculiar high mass X-ray binary with a main-sequence donor star. Recent X-ray observations suggested that the compact object in 4U 2206+54 may be a neutron star. The X-ray emission comes from the accretion of stellar winds from the massive donor stars, and variability of luminosity may be due to the changes of its orbit phase. To further reveal the nature of compact object, we studied 4U 2206+54 with INTEGRAL/IBIS observations in two years, and found that in most time, 4U 2206+54 undergone a quiescent state and sometime an active state. In the quiescent state the spectrum can be fitted by a power-law model of $Γ\sim 2.1$ with a hard X-ray luminosity of $\sim 5\times 10^{34}$ erg s$^{-1}$ (20-- 100 keV). While in the active state, the 20-- 100 keV hard X-ray luminosity reaches $\sim 2\times 10^{35}$ erg s$^{-1}$ and the spectrum is fitted by a thermal bremmstrahlung model of $kT\sim 43$ keV plus two cyclotron absorption lines at $\sim$ 30 and 60 keV. Then we derived a magnetic field of 3.3$\times 10^{12}$ G for the compact object in 4U 2206+54. During the active state, we found a pulsation period of $\sim$ 5400 s in the light curve of 4U 2206+54. So the compact object in 4U 2206+54 should be a magnetic neutron star with a slow pulsation. Cyclotron absorption lines detected in the active state and non-detection in the quiescent state suggested that two different accretion states have possible different hard X-ray emission regions: surface of neutron star in the active state; the magnetic-accretion pressure equivalent point in the quiescent state. The re-analysis of the RXTE/ASM light curve found the modulation periods at $\sim 9.56$ days and 19.11 days, and the orbit period of 4U 2206+54 should be 19.11 days.
description: 7 pages, 8 figures, 1 table, MNRAS in press
Blazar 3C 454.3 in Outburst and Quiescence During 2005-2007: Two Variable Synchrotron Emission Peaks
Creators: name: Ogle, Patrick M.
name: Wehrle, Ann E.
name: Balonek, Thomas
name: Gurwell, Mark A.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We monitored the flaring blazar 3C 454.3 during 2005 June-July with the Spitzer Infrared Spectrograph (IRS: 15 epochs), Infrared Array Camera (IRAC: 12 epochs) and Multiband Imaging Photometer (MIPS: 2 epochs). We also made Spitzer IRS, IRAC, and MIPS observations from 2006 December-2007 January when the source was in a low state, the latter simultaneous with a single Chandra X-ray observation. In addition, we present optical and sub-mm monitoring data. The 2005-2007 period saw 3 major outbursts. We present evidence that the radio-optical SED actually consists of two variable synchrotron peaks, the primary at IR and the secondary at sub-mm wavelengths. The lag between the optical and sub-mm outbursts may indicate that these two peaks arise from two distinct regions along the jet separated by a distance of 0.07-5 pc. The flux at 5-35 microns varied by a factor of 40 and the IR peak varied in frequency from <1E13 Hz to 4E13 Hz between the highest and lowest states in 2005 and 2006, respectively. Variability was well correlated across the mid-IR band, with no measurable lag. Flares that doubled in flux occurred on a time scale of 3 days. The IR SED peak moved to higher frequency as a flare brightened, then returned to lower frequency as it decayed. The fractional variability amplitude increased with frequency, which we attribute to decreasing synchrotron-self absorption optical depth. Mid-IR flares may signal the re-energization of a shock that runs into inhomogeneities along the pre-existing jet or in the external medium. The synchrotron peak frequencies during each major outburst may depend upon both the distance from the jet apex and the physical conditions in the shocks. Variation of the Doppler parameter along a curved or helical jet is another possibility. Frequency variability of the IR synchrotron peak may have important consequences for the interpretation of the blazar sequence, and the presence of a secondary peak may give insight into jet structure.
description: 38 pages, 15 figures, submitted to ApJS, comments welcome
title: Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ°ÑÑÑ Ð¢Ð­Ð¦ Ñ Ð´Ð²ÑÐ¼Ñ ÑÐ½ÐµÑÐ³Ð¾Ð±Ð»Ð¾ÐºÐ°Ð¼Ð¸ ÐÐÐ£-200
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÑÐ¸Ð¾Ð½Ð°ÐºÐ¸Ñ, ÐÐ¸ÑÐ°Ð¸Ð»
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð¢ÐµÐ¿Ð»Ð¾Ð²ÑÐµ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÑÐ°Ð½ÑÐ¸Ð¸
Ð¢Ð¾ÐºÐ¸ ÐºÐ¾ÑÐ¾ÑÐºÐ¾Ð³Ð¾ Ð·Ð°Ð¼ÑÐºÐ°Ð½Ð¸Ñ
ÐÐµÐ½ÐµÑÐ°ÑÐ¾ÑÑ
Ð¢ÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð°ÑÐ¾ÑÑ

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ°ÑÑÐ¸ ÑÐ»ÐµÐºÑÑÐ¾ÑÑÐ°Ð½ÑÐ¸Ð¸. ÐÑÐ±ÑÐ°Ð½Ð° Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð°Ñ ÑÑÑÑÐºÑÑÑÐ½Ð°Ñ ÑÑÐµÐ¼Ð° Ð¸ Ð¾ÑÐ½Ð¾Ð²Ð½Ð¾Ðµ ÑÐ»ÐµÐºÑÑÐ¾Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ñ ÑÐ¾ÐºÐ¸ ÐºÐ¾ÑÐ¾ÑÐºÐ¾Ð³Ð¾ Ð·Ð°Ð¼ÑÐºÐ°Ð½Ð¸Ñ. ÐÑÐ±ÑÐ°Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÑ Ð¸ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¸ÐºÐ¸. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð³Ð»Ð°Ð²Ð½Ð°Ñ ÑÑÐµÐ¼Ð° ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ð¹ Ð¸ ÑÑÐµÐ¼Ð° ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð½ÑÐ¶Ð´.
Roman2020 conference schedule: "Galaxy Formation and Evolution in the Era of the Nancy Grace Roman Space Telescope"
Creators: name: Ryan, Russell
name: Deustua, Susana
name: Hathi, Nimish
name: Mutchler, Max
Publisher: name: Zenodo
Year: 2020

description: Our knowledge of galaxy formation and evolution has greatly expanded in recent decades thanks to large survey programs, including those carried out with the Hubble Space Telescope (HST). These programs led to numerous discoveries, deepening our understanding of the properties of high-redshift galaxies, the evolution of galaxy morphology over cosmic time, the physics of quenching and feedback mechanisms, populations of faint or optically obscured AGN, and enabled a new era of multi-wavelength photometric redshifts. But, to significantly further advance in the future, we need to expand our observations to exploit wide-field capabilities, beyond HST's relatively narrow sky coverage, in the next decade of surveys with upcoming facilities such as the James Webb Space Telescope, the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST), the Euclid Mission and the Nancy Grace Roman Space Telescope, formerly named the Wide Field Infrared Survey Telescope (WFIRST). Specifically, the Roman Space Telescope, planned for launch in the mid-2020s, will provide HST quality imaging over 0.28 sq. degrees (a field of view about a 100x larger than HST/ACS) at wavelengths between 0.5 microns and 2 microns. In addition to performing dedicated surveys, the Roman Space Telescope will support a Guest Observer program and archival investigations of all Roman data, which will be open to the community with no proprietary period. Roman’s large field of view will enable vastly larger galaxy surveys than possible with HST. This conference aims to engage the extragalactic community in exploring how we can synergistically advance the astrophysics of galaxy formation and evolution in the era of the Nancy Grace Roman Space Telescope.
Probing the interface of Fe3O4/GaAs thin films by hard x-ray photoelectron spectroscopy
Creators: name: Paul, M.
name: Mueller, A.
name: Ruff, A.
name: Schmid, B.
name: Berner, G.
name: Mertin, M.
name: Sing, M.
name: Claessen, R.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Magnetite (Fe3O4) thin films on GaAs have been studied with HArd X-ray PhotoElectron Spectroscopy (HAXPES) and low-energy electron diffraction. Films prepared under different growth conditions are compared with respect to stoichiometry, oxidation, and chemical nature. Employing the considerably enhanced probing depth of HAXPES as compared to conventional x-ray photoelectron spectroscopy (XPS) allows us to investigate the chemical state of the film-substrate interfaces. The degree of oxidation and intermixing at the interface are dependent on the applied growth conditions; in particular, we found that metallic Fe, As2O3, and Ga2O3 exist at the interface. These interface phases might be detrimental for spin injection from magnetite into GaAs.
description: 5 pages, 3 figures
Recruitment of curling pebbles during repeated passes of a curling stone
Creators: name: Maw, Sean
name: Harris, Grant
name: Sharbel, Lara
name: Hritzuk, Eugene
Publisher: name: Loughborough University
Year: 2024

description: Engineering of Sport 15 - Proceedings from the 15th International Conference on the Engineering of Sport (ISEA 2024)

In the winter sport of curling, curling stones glide over carefully prepared ice. Water droplets are sprayed over the ice and most freeze into circular cones which are colloquially known as “pebbles”. Pebbles come in various sizes and heights and oftentimes before a competition they will be “nipped”. This means that a sharp edge will be dragged over the ice surface to truncate the conic pebbles. Once this is done, the ice is ready for curling. As curling stones repeatedly pass over the nipped pebbles, the pebbles slowly change. Ice is gradually shaved off the tops of the pebbles. This results in two distinct effects: the tops of the nipped pebbles increase in area, and as the tops get shaved, new (shorter) pebbles are “recruited” and become truncated cones themselves. This is important in curling because this gradually increasing surface area over which the stones glide is the primary source of increasing dynamic friction forces that the curling stones experience. As the pebbles change, so do the playing conditions. Characterizing these changes can help competitors as well as ice technicians. It may also help further the understanding of the physics driving the “curl” in curling. Prior to this study, the temporal changes in the nature of the pebbles had not been characterized in any detail.
Narrowband tunable filter based on velocity-selective optical pumping in an atomic vapor
Creators: name: Cere, Alessandro
name: Parigi, Valentina
name: Abad, Marta
name: Wolfgramm, Florian
name: Predojevic, Ana
name: Mitchell, Morgan W.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We demonstrate a tunable, narrow-band filter based on optical-pumping-induced circular dichroism in rubidium vapor. The filter achieves a peak transmission of 14.6%, a linewidth of 80 MHz, and an out-of-band extinction >35 dB. The transmission peak can be tuned within the range of the Doppler linewidth of the D1 line of atomic rubidium at 795 nm. While other atomic filters work at frequencies far from absorption, the presented technique provides light resonant with atomic media, useful for atom-photon interaction experiments. The technique could readily be extended to other alkali atoms.
description: 3 Pages, 4 figures
Stemonitopsis typhina var. similis  Nann.- Bremek. & Y. Yamam
Creators: name: Kluša, Julita
Publisher: name: Zenodo
Year: 2023
Subjects: Biodiversity
Taxonomy
Protozoa
Mycetozoa
Myxomycetes
Stemonitidales
Stemonitidaceae
Stemonitopsis
Stemonitopsis typhina

description: ● Stemonitopsis typhina (F.H. Wigg.) Nann.- Bremek. var. similis (G. Lister) Nann.- Bremek. & Y. Yamam.,
līdzīgā cilindrīte
- leg. A.Piroga, 12 Jul 2023, Arona p., on the soil, possibly on heavily decomposed wood remains, det. J. Kluša, 2023; (JK), very rare.
description: Published as part of Kluša, Julita, 2023, Complete Checklist Of Myxomycetes In Latvia, pp. 127-151 in Acta Biologica Universitatis Daugavpiliensis 23 (2) on pages 127-151, DOI: 10.59893/abud.23(2).002, http://zenodo.org/record/12650118
Dreaming, speculating, imagining otherwise : radical spacetime imaginaries in postcolonial speculative comics
Creators: name: Chatterjee, Meghna
Publisher: name: University of British Columbia
Year: 2024

description: This thesis investigates the futures imagined by exilic figures in postcolonial speculative graphic fiction. Sarterp Namiq et al.’s Temple of Refuge features an unnamed Kurdish refugee envisioning new futures post-displacement, while Bishakh Som’s Swandive follows two gender nonconforming Bengali Americans grappling with their place in the world. Mobilizing the theoretical apparatuses of formalist comics studies, speculative fiction studies, and critical race and gender studies, this thesis explores how the comic form’s ability to reimagine and materialize new realities engages with debates on speculative thinking and lifemaking in the postcolonial context. Chapter 1 examines the formation of the exilic figure in Temple of Refuge and Swandive. Here, “exile” is used to denote a psychological state of being “unmoored,” fostering the creation of “imaginary homelands” (Rushdie) and “oddkin” communities (Haraway). I theorize the exilic figure through the heuristic of exilic rupture, or the emotional and affective disjunct that tethers the exile from rationalist understanding of space and time. Chapter 2 delves into the comic form's support of the exilic imagination. I examine how the aesthetic strategies of both texts demonstrate exilic rupture, particularly how the Temple of Refuge employs the aesthetic of the photo album to bring spatiotemporal confusion into focus. I also look at how the gutterless pages of Swandive spur into life an imagined world of the exile. The thesis concludes with a Coda reflecting on the concept of bearing witness in speculative fiction and the implications of comic visualization for forming an "implicated subject." It raises questions about ethics, politics, and responsibility, exploring how the “ethics and politics of recognition” (Whitlock) transform when realism yields to speculation. By reading the comic page as an expression of precarious imaginaries, this thesis opens inquiries into the reader's role in supporting non-hegemonic visual cultures.
ByzRev 03.2021.005: Symeon Tsolakidis (Hg.), Die Chronik von Morea. Übersetzt, eingeleitet und mit Anmerkungen versehen
Creators: name: Makris, Georgios
Publisher: name: The Byzantine Review
Year: 2021

description: Symeon Tsolakidis (Hg.), Die Chronik von Morea. Übersetzt, eingeleitet und mit Anmerkungen versehen (Studien zur Orientalischen Kirchengeschichte 57). Berlin: LIT Verlag Dr. W. Hopf 2019. 342 S. – ISBN: 978-3-643-14057-9 (€ 34,90)
description: The Byzantine Review, Bd. 3 (2021)
title: ÐÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐµÐ½Ð½Ð¾ÑÑÐ½ÑÑ Ð¾ÑÐ¸ÐµÐ½ÑÐ°ÑÐ¸Ð¹ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÐ·Ð°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¯ÐºÐ¾Ð²Ð»ÐµÐ²Ð°, ÐÐµÑÐ¾Ð½Ð¸ÐºÐ°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÑÐµÐ½Ð½Ð¾ÑÑÑ
ÑÐµÐ½Ð½Ð¾ÑÑÐ½ÑÐµ Ð¾ÑÐ¸ÐµÐ½ÑÐ°ÑÐ¸Ð¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð²
ÑÐ¸ÑÑÐµÐ¼Ð° ÑÐµÐ½Ð½Ð¾ÑÑÐµÐ¹
Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð°Ñ ÑÑÐµÐ´Ð°

description: Ð¦ÐµÐ»ÑÑ Ð½Ð°ÑÑÐ¾ÑÑÐµÐ³Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐµÐ¹ ÑÐµÐ½Ð½Ð¾ÑÑÐ½ÑÑ Ð¾ÑÐ¸ÐµÐ½ÑÐ°ÑÐ¸Ð¹ Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¿ÐµÑÐ²Ð¾Ð³Ð¾ Ð¸ ÑÐµÑÐ²ÐµÑÑÐ¾Ð³Ð¾ ÐºÑÑÑÐ¾Ð² Ð³ÑÐ¼Ð°Ð½Ð¸ÑÐ°ÑÐ½Ð¾Ð³Ð¾ Ð¸Ð½ÑÑÐ¸ÑÑÑÐ° Ð¡ÐÐÐÐ£. ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð²ÐºÐ»ÑÑÐ°ÐµÑ Ð² ÑÐµÐ±Ñ Ð´Ð²Ðµ Ð³Ð»Ð°Ð²Ñ - ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÑÑ Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÑÑ. Ð Ð¿ÐµÑÐ²Ð¾Ð¹ Ð³Ð»Ð°Ð²Ðµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ Ð¿Ð¾Ð´ÑÐ¾Ð´Ñ Ðº Ð¿Ð¾Ð½Ð¸Ð¼Ð°Ð½Ð¸Ñ Ð¿Ð¾Ð½ÑÑÐ¸Ð¹ Â«ÑÐµÐ½Ð½Ð¾ÑÑÑÂ» Ð¸ Â«ÑÐµÐ½Ð½Ð¾ÑÑÐ½ÑÐµ Ð¾ÑÐ¸ÐµÐ½ÑÐ°ÑÐ¸Ð¸Â» Ð² ÑÐ¸Ð»Ð¾ÑÐ¾ÑÐ¸Ð¸, Ð¿ÑÐ¸ÑÐ¾Ð»Ð¾Ð³Ð¸Ð¸, ÑÐ¾ÑÐ¸Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸ Ð¿ÐµÐ´Ð°Ð³Ð¾Ð³Ð¸ÐºÐµ, Ð¸Ð·ÑÑÐµÐ½Ð° Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð° ÑÐ¾Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ Ð´Ð°Ð½Ð½ÑÑ Ð¿Ð¾Ð½ÑÑÐ¸Ð¹, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½ ÑÑÑÐ´ÐµÐ½ÑÐµÑÐºÐ¸Ð¹ Ð²Ð¾Ð·ÑÐ°ÑÑ ÐºÐ°Ðº ÑÐµÐ½Ð·Ð¸ÑÐ¸Ð²Ð½ÑÐ¹ Ð¿ÐµÑÐ¸Ð¾Ð´ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÐ½Ð½Ð¾ÑÑÐµÐ¹ Ð¸ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð°Ñ ÑÑÐµÐ´Ð° ÐºÐ°Ðº ÑÐ°ÐºÑÐ¾Ñ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐµÐ½Ð½Ð¾ÑÑÐ½ÑÑ Ð¾ÑÐ¸ÐµÐ½ÑÐ°ÑÐ¸Ð¹ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð². Ð Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð³Ð»Ð°Ð²Ðµ ÑÐ´ÐµÐ»Ð°Ð½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¾Ð¿ÑÐ¾ÑÐ° ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¿ÐµÑÐ²Ð¾Ð³Ð¾ Ð¸ ÑÐµÑÐ²ÐµÑÑÐ¾Ð³Ð¾ ÐºÑÑÑÐ¾Ð² Ð¿Ð¾ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐµ Ð. Ð Ð¾ÐºÐ¸ÑÐ°. ÐÑÐ¸ Ð½Ð°Ð¿Ð¸ÑÐ°Ð½Ð¸Ð¸ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ñ ÑÐ»ÐµÐ´ÑÑÑÐ¸Ðµ Ð¼ÐµÑÐ¾Ð´Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ: Ð°Ð½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ð¹, ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð¸ Ð´Ð¸Ð°Ð³Ð½Ð¾ÑÑÐ¸ÑÐµÑÐºÐ¸Ð¹. ÐÐ±Ð»Ð°ÑÑÑ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ: Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÐµ Ð´Ð°Ð½Ð½ÑÐµ Ð¼Ð¾Ð³ÑÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ñ Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÑÐ¼Ð¸ Ð´Ð»Ñ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÐ½Ð½Ð¾ÑÑÐ½ÑÑ Ð¾ÑÐ¸ÐµÐ½ÑÐ°ÑÐ¸Ð¹ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÐÑÐ¼Ð°Ð½Ð¸ÑÐ°ÑÐ½Ð¾Ð³Ð¾ Ð¸Ð½ÑÑÐ¸ÑÑÑÐ° Ð¸ Ð´Ð»Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÑÐµÐ±Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ°.
title: ÐÐ´Ð¾ÑÐ¾Ð²ÑÐµ - Ð¾ÑÐ½Ð¾Ð²Ð° ÑÐµÐ»Ð¾Ð²ÐµÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»Ð°: Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¸ Ð¿ÑÑÐ¸ Ð¸Ñ ÑÐµÑÐµÐ½Ð¸Ñ
title: ÑÑÑÐ´Ñ ÐÑÐµÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð½Ð°ÑÑÐ½Ð¾Ð¹ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ð¸, 26-28 ÑÐµÐ½ÑÑÐ±ÑÑ 2006 Ð³.
titleType: Subtitle
Creators: name: "ÐÐ´Ð¾ÑÐ¾Ð²ÑÐµ-Ð¾ÑÐ½Ð¾Ð²Ð° ÑÐµÐ»Ð¾Ð²ÐµÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»Ð°: Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¸ Ð¿ÑÑÐ¸ Ð¸Ñ  ÑÐµÑÐµÐ½Ð¸Ñ", Ð²ÑÐµÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ°Ñ Ð½Ð°ÑÑÐ½Ð°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (2006; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2006
Subjects: Ð·Ð´Ð¾ÑÐ¾Ð²ÑÐµ
Ð·Ð°Ð±Ð¾Ð»ÐµÐ²Ð°ÐµÐ¼Ð¾ÑÑÑ
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description: Ð ÐºÐ½Ð¸Ð³Ðµ Ð¾Ð¿ÑÐ±Ð»Ð¸ÐºÐ¾Ð²Ð°Ð½Ñ ÐÑÐ¾Ð³Ð¾Ð²ÑÐ¹ Ð´Ð¾ÐºÑÐ¼ÐµÐ½Ñ Ð¸ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ ÐÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ð¸, ÑÐµÐ·Ð¸ÑÑ Ð´Ð¾ÐºÐ»Ð°Ð´Ð¾Ð² Ð¸ ÑÑÐ°ÑÐµÐ¹, Ð¾ÑÑÐ°Ð¶Ð°ÑÑÐ¸Ñ ÑÑÐ¾Ð²ÐµÐ½Ñ Ð¸ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÑ Ð·Ð°Ð±Ð¾Ð»ÐµÐ²Ð°ÐµÐ¼Ð¾ÑÑÐ¸ Ð¿Ð¾ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐ¼ Ð³ÑÑÐ¿Ð¿Ð°Ð¼ Ð·Ð°Ð±Ð¾Ð»ÐµÐ²Ð°Ð½Ð¸Ð¹, ÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð¶Ð´Ð°ÑÑÐ¸ÑÑÑ ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸ÐµÐ¼ ÑÐ¼ÐµÑÑÐ½Ð¾ÑÑÐ¸ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸Ñ. ÐÑÐ¸Ð²Ð¾Ð´ÑÑÑÑ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¾ Ð´ÐµÐ¼Ð¾Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ°Ñ Ð² Ð½Ð°ÑÐµÐ¹ ÑÑÑÐ°Ð½Ðµ. ÐÑÐµÐ´Ð»Ð°Ð³Ð°ÑÑÑÑ Ð¿ÑÑÐ¸ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ Ð·Ð´Ð¾ÑÐ¾Ð²ÑÑ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸Ñ Ð² ÑÑÑÐ°Ð½Ðµ Ð¸ ÐµÐµ Ð¾ÑÐ´ÐµÐ»ÑÐ½ÑÑ ÑÐµÐ³Ð¸Ð¾Ð½Ð°Ñ, Ð³Ð¾ÑÐ¾Ð´Ð°Ñ Ð¸ ÑÑÑÐµÐ¶Ð´ÐµÐ½Ð¸ÑÑ.
Dynamics of Chemical Equilibrium of Hadronic Matter Close to $T_c$
Creators: name: Noronha-Hostler, J.
name: Beitel, M.
name: Greiner, C.
name: Shovkovy, I.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Quick chemical equilibration times of hadrons (specifically, $p\bar{p}$, $K\bar{K}$, $Λ\barΛ$, and $Ω\barΩ$ pairs) within a hadron gas are explained dynamically using Hagedorn states, which drive particles into equilibrium close to the critical temperature. Within this scheme, we use master equations and derive various analytical estimates for the chemical equilibration times. We compare our model to recent lattice results and find that for both $T_c=176$ MeV and $T_c=196$ MeV, the hadrons can reach chemical equilibrium almost immediately, well before the chemical freeze-out temperatures found in thermal fits for a hadron gas without Hagedorn states. Furthermore the ratios $p/π$, $K/π$, $Λ/π$, and $Ω/ π$ match experimental values well in our dynamical scenario.
description: 20 pages, 56 figures
Farming Alternatives for Potato Growers on the Eastern Shore (Virginia-Maryland)
Creators: name: Strand, Edwin G.
name: Strand, Edwin G.
Publisher: name: Unknown
Year: 1953
Subjects: subject: Crop Production/Industries
subject: Farm Management
subject: Marketing
subject: FOS: Economics and business
subject: Production Economics
subject: Research and Development/Tech Change/Emerging Technologies

description: Excerpt from the report Introduction: In recent years potato growers have been faced with a serious problem of adjustment. Improved technology as applied to production of potatoes has increased yields per acre more than for most crops. At the same time, per capita consumption of potatoes has steadily declined. A smaller acreage of this crop is needed and alternative crops must be found to make up a well-balanced farming system. Desirable farming alternatives depend on the special circumstances of different areas. The purpose of this study Is to analyze the alternatives available in an area in which a marked shift in acreage has already taken place and in which further changes may be necessary. In this report the situation relating to small and medium-sized farms is emphasized. These farms constitute the large majority in the area and ordinarily they have the most acute problems of adjustment in maintaining or Improving farm incomes.
title: ÐÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ðµ ÑÑÑÐ°Ñ Ð¾Ð²Ð°Ð½Ð¸Ðµ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐµÑÑÐ½Ð¾Ð²Ð°, ÐÐ°ÑÐ°Ð»ÑÑ
name: ÐÐ¾Ð¿Ð¾Ð²Ð°, ÐÐ»ÑÐ³Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÑÑÑÐ°Ñ Ð¾Ð²Ð°Ð½Ð¸Ðµ
ÑÑÑÐ°Ñ Ð¾Ð²ÑÐµ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸
ÑÑÑÐ°Ñ Ð¾Ð²ÑÐµ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¸

description: Ð¡Ð¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¼Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¼Ñ ÑÑÐ°Ð½Ð´Ð°ÑÑÑ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ 080200.62 Â«ÐÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÂ». ÐÐ·Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð° Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ, Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ðº ÑÐºÐ·Ð°Ð¼ÐµÐ½Ñ, Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ð¿Ð¾ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÐºÑÑÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ°. Ð ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÐ±Ð¾ÑÐ½Ð¸Ðº Ð·Ð°Ð´Ð°Ñ Ð¿Ð¾ ÑÐµÐ¼Ð°Ð¼ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ, Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ð¿Ð¾ Ð¸Ñ ÑÐµÑÐµÐ½Ð¸Ñ, ÑÐµÐ¼Ñ ÑÐµÑÐµÑÐ°ÑÐ¾Ð² Ð´Ð»Ñ ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ, Ð²Ð°ÑÐ¸Ð°Ð½ÑÑ ÑÐµÑÑÐ¾Ð² Ð¸ ÐºÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½ÑÑ ÑÐ°Ð±Ð¾Ñ Ð´Ð»Ñ ÑÐµÐºÑÑÐµÐ³Ð¾ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ Ð·Ð½Ð°Ð½Ð¸Ð¹, Ð³Ð»Ð¾ÑÑÐ°ÑÐ¸Ð¹. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ 38.03.02 -Â«ÐÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÂ», 38.03.02.09 - Â«ÐÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð°Ñ Ð»Ð¾Ð³Ð¸ÑÑÐ¸ÐºÐ°Â» ÐÐ½ÑÑÐ¸ÑÑÑÐ° Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÐ°, ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ Ð¸ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸. ÐÐ¾Ð³ÑÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ñ ÑÐ°ÐºÐ¶Ðµ ÑÐ»ÑÑÐ°ÑÐµÐ»ÑÐ¼Ð¸ Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹ Ð¿Ð¾ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÑ.
A peculiar HI cloud near the distant globular cluster Pal 4
Creators: name: van Loon, Jacco Th.
name: Stanimirovic, Snezana
name: Putman, Mary
name: Peek, Joshua E. G.
name: Gibson, Steven J.
name: Douglas, Kevin A.
name: Korpela, Eric J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present 21-cm observations of four Galactic globular clusters, as part of the on-going GALFA-HI Survey at Arecibo. We discovered a peculiar HI cloud in the vicinity of the distant (109 kpc) cluster Pal 4, and discuss its properties and likelihood of association with the cluster. We conclude that an association of the HI cloud and Pal 4 is possible, but that a chance coincidence between Pal 4 and a nearby compact high-velocity cloud cannot be ruled out altogether. New, more stringent upper limits were derived for the other three clusters: M 3, NGC 5466, and Pal 13. We briefly discuss the fate of globular cluster gas and the interaction of compact clouds with the Galactic Halo gas.
description: Accepted for publication in MNRAS