bluuebunny/crossref_metadata_2025_split huggingface dataset:
PERCOBAAN PEMBUNUHAN SEBAGAI PENGHALANG HAK WARIS PERSPEKTIF HUKUM ISLAM DAN KOMPILASI HUKUM ISLAM
Authors: Khisni Akhmad , Ulinnuha M 
Published: July 2017

ABSTRACTIn terms of the obstruction of the right of inheritance for the crime of attempted murder of a conflict between Islamic Law and Islamic Law Compilation (KHI). In Islamic law, which was the cause of obstruction of the right of inheritance is someone for murder, slavery, religious differences, and different countries. In conditions that are not elements of the crime of attempted murder as the cause of obstruction of an inheritance. This provision departs from the principle of law in Islamic law regarding jarimah completed the murder and no jarimah / pending (attempted murder).On the other hand, clearly states KHI jarimah attempted murder is the element that causes obstruction of the right of inheritance as a provision contained in Article 173 KHI. Thus visible difference between the provisions of Islamic law and KHI, which has been placed as the provisions of Islamic law for the people of Indonesia. To address the problem, the authors use the research methods of law with juridical-normative legal research conducted by prioritizing research library materials or documents referred to secondary data, in the form of legal materials, primary and secondary. Specifications research is descriptive, which aims to give an overview conducted by way of qualitative theories of law and legal doctrine, and expert opinion of Islamic law.In conclusion, between Islamic law and there is no difference KHI opposite each other with respect to the legal principles adopted by each. The provisions in Article 173 KHI can be filed as a realization of the principles of Islamic law in the delivery of a legal provision will be enforced to have known it, or judge to determine the sentence for the crime ta'zir (jarimah). Conditions resulting known it, or judge it to be established in the form of a regulatory law that was born because of judicial decisions (jurisprudence), which in this case is the provision of an obstruction of the right of inheritance for reasons of criminal offenses of attempted murder.
PERUBAHAN SISTEM HUKUM MENUJU JATI DIRI SEBUAH NEGARA
Authors: Abra Emy Hajar 
Published: July 2017

Legal system of a state determine the main source of law in making a legal policy, clearly legal systems has certain characteristic although on the development differences among legal system cannot be seen clearly.To comprehend and strengthen the legal systemof a staterequired an observation toward legal system of other states as comparison. The function of legal systems comparison is the basis to grouping states into the family of legal system.Basically legal system describes legal form of a state, hence when a legal system createdfrom structure, substance and culture of certain state the legal system must reflect the state identity. Several factors influence the process to develop a legal system, such as economics, political and social. Means, legal system could be form not only by internal values but also external factorsof state. As a result to avoid legal systems with thin similarities and differences, finding a suitable legal system that in line with the identity of a country is a better way.Discussion about the thin differences between Continental European and Anglo-Saxon do not get big attention as before, impressed ignored and turn out trigger of questions. Why a stateunable to consistently espoused the legal system?, whethergrouping legal systemsinto family of legal system no longer important?. This paper will answer those question by deeply examinethe restorationof legal system so that in line with the historical value of a state. Colonized states often apply legal system that comes from colonizer after independent which means their legal system is notthe state pure legal system that can be incompatible with the values that develop in a state. Would be inconsistent when the legal system applied is Continental European, but in fact the values, laws, institutions and legal verdict are based on the values of religious, Islam for instance.Gambia,a state in Africa with 95% of population is Muslim and the former British colonytake a big step by leave the legacy of colonial legal system, Anglo-Saxon. Gambia. How could a state forced to follow the legal systems of other states remember law is an independent rule, free from interference and coercion. This is the focus study will explain about that when legal system with openness value must have consistency with values that recognizedand upheld by society in a state. As a result changes in a legal system toward identity of a country are necessity and inevitable. On the other hand, debates and critics on the thin differences of legal system should be an independent study to discuss.
HPLC analysis, anti-oxidant activity of Genista ferox and its anti-proliferative effect in HeLa cell line
Authors: Bencherchar Ilhem , Demirtas Ibrahim , Altun Muhammed , Gul Fatih , Sarri Djamel , Benayache Fadila , Benayache Samir , Mekkiou Ratiba 
Published: July 2017

The prevention and treatment of the cancer using plants have attracted increasing interest. The present study was aimed to determine the phenolic compounds of Genista ferox using HPLC-TOF/MS and the anti-oxidant acti-vity associated with anti-cancer activity against human cervical adenocarcinoma (HeLa) cell line. Total anti-oxidant capacities of different extracts of G. ferox were assessed by DPPH assay, and their total phenolic and flavonoids contents measured by FolinCiocalteu and aluminum trichloride assays. The amounts of total phenolic (105.2 ± 0.6  308.5 ± 5.7 mg/g) of extract measured as gallic acid equivalent and flavonoids (8.1 ± 0.1  124.0 ± 0.7 mg/g) of extract measured as quercetin equivalent varied from chloroform to n-butanol extract of the two parts of the plant (leaf and stem). The ethyl acetate extract of G. ferox exhibited the most powerful effect on the DPPH scavenging activity with 94% from the leaf and 93% from the stem, while the chloroform extract from the leaf exhibited the most effective anti-proliferative activity against HeLa cell lines.
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Vascular development in very young conifer seedlings: Theoretical hydraulic capacities and potential resistance to embolism
Authors: Miller Megan L. , Johnson Daniel M. 
Published: July 2017

PREMISE OF THE STUDY:Conifers have the highest rates of mortality during their first year, often attributed to water stress; yet, this tree life stage is the least studied in terms of hydraulic properties. Previous work has revealed correlations between xylem anatomy to both hydraulic transport capacity and resistance to hydraulic dysfunction. In this study, we compared xylem anatomical and plant functional traits of Pseudotsuga menziesii, Larix occidentalis, and Pinus ponderosa seedlings over the first 10 wk of growth to evaluate potential maximum hydraulic capabilities and resistance to drought‐induced embolism. We hypothesized that, based on key functional traits of the xylem, predicted xylem embolism resistance of the species will reflect their previously determined drought tolerances with L. occidentalis, P. menziesii, and P. ponderosa in order of least to most embolism‐resistant xylem.METHODS:Xylem and pit anatomical characteristics and additional hydraulic‐related functional traits were compared at five times during the first 10 wk of growth using confocal laser scanning microscopy (CLSM).KEY RESULTS:Based on thickness to span ratio, torus to pit aperture overlap, and torus thickness, primary xylem appeared to be not only more hydraulically conductive but also less embolism‐resistant than secondary xylem. By week 10, P. menziesii was predicted to have the most embolism‐resistant xylem followed by P. ponderosa and L. occidentalis.CONCLUSIONS:Theoretical measurements suggest that hydraulic transport capacities and vulnerability to embolism varied for each species over the first 10 wk of growth; thus, the timing of germination and onset of limited soil moisture is critical for growth and survival of seedlings.
First Large-scale Herbig–Haro Jet Driven by a Proto-brown Dwarf
Authors: Riaz B. , Briceño C. , Whelan E. T. , Heathcote S. 
Published: July 2017

Abstract
We report the discovery of a new Herbig–Haro jet, HH 1165, in SOAR narrow-band imaging of the vicinity of the σ Orionis cluster. HH 1165 shows a spectacular extended and collimated spatial structure, with a projected length of 0.26 pc, a bent C-shaped morphology, multiple knots, and fragmented bow shocks at the apparent ends of the flow. The Hα image shows a bright halo with a clumpy distribution of material seen around the driving source, and curved reflection nebulosity tracing the outflow cavities. The driving source of HH 1165 is a Class I proto-brown dwarf, Mayrit 1701117 (M1701117), with a total (dust+gas) mass of ∼36 M
Jup and a bolometric luminosity of ∼0.1 L
⊙. High-resolution VLT/UVES spectra of M1701117 show a wealth of emission lines indicative of strong outflow and accretion activity. SOAR/Goodman low-resolution spectra along the jet axis show an asymmetrical morphology for HH 1165. We find a puzzling picture wherein the northwest part exhibits a classical HH jet running into a pre-dominantly neutral medium, while the southern part resembles an externally irradiated jet. The C-shaped bending in HH 1165 may be produced by the combined effects from the massive stars in the ionization front to the east, the σ Orionis core to the west, and the close proximity to the B2-type star HR 1950. HH 1165 shows all of the signatures to be considered as a scaled-down version of parsec-length HH jets, and can be termed as the first sub-stellar analog of a protostellar HH jet system.
iPTF16fnl: A Faint and Fast Tidal Disruption Event in an E+A Galaxy
Authors: Blagorodnova N. , Gezari S. , Hung T. , Kulkarni S. R. , Cenko S. B. , Pasham D. R. , Yan L. , Arcavi I. , Ben-Ami S. , Bue B. D. , Cantwell T. , Cao Y. , Castro-Tirado A. J. , Fender R. , Fremling C. , Gal-Yam A. , Ho A. Y. Q. , Horesh A. , Hosseinzadeh G. , Kasliwal M. M. , Kong A. K. H. , Laher R. R. , Leloudas G. , Lunnan R. , Masci F. J. , Mooley K. , Neill J. D. , Nugent P. , Powell M. , Valeev A. F. , Vreeswijk P. M. , Walters R. , Wozniak P. 
Published: July 2017

Abstract
We present ground-based and Swift observations of iPTF16fnl, a likely tidal disruption event (TDE) discovered by the intermediate Palomar Transient Factory (iPTF) survey at 66.6 Mpc. The light curve of the object peaked at an absolute mag

. The maximum bolometric luminosity (from optical and UV) was

erg s−1, an order of magnitude fainter than any other optical TDE discovered so far. The luminosity in the first 60 days is consistent with an exponential decay, with

, where t
0 = 57631.0 (MJD) and

days. The X-ray shows a marginal detection at

erg s−1 (Swift X-ray Telescope). No radio counterpart was detected down to 3σ, providing upper limits for monochromatic radio luminosities of

erg s−1 and

erg s−1 (Very Large Array, 6.1 and 22 GHz). The blackbody temperature, obtained from combined Swift UV and optical photometry, shows a constant value of 19,000 K. The transient spectrum at peak is characterized by broad He ii and Hα emission lines, with FWHMs of about 14,000 km s−1 and 10,000 km s−1, respectively. He i lines are also detected at λλ 5875 and 6678. The spectrum of the host is dominated by strong Balmer absorption lines, which are consistent with a post-starburst (E+A) galaxy with an age of ∼650 Myr and solar metallicity. The characteristics of iPTF16fnl make it an outlier on both luminosity and decay timescales, as compared to other optically selected TDEs. The discovery of such a faint optical event suggests a higher rate of tidal disruptions, as low-luminosity events may have gone unnoticed in previous searches.
MHOs toward HMOs: A Search for Molecular Hydrogen Emission-Line Objects toward High-mass Outflows
Authors: Wolf-Chase Grace , Arvidsson Kim , Smutko Michael 
Published: July 2017

Abstract
We present the results of a narrow-band near-infrared imaging survey for Molecular Hydrogen emission-line Objects (MHOs) toward 26 regions containing high-mass protostellar candidates and massive molecular outflows. We have detected a total of 236 MHOs, 156 of which are new detections, in 22 out of the 26 regions. We use H2 2.12 μm/H2 2.25 μm flux ratios, together with morphology, to separate the signatures of fluorescence associated with photo-dissociation regions (PDRs) from shocks associated with outflows in order to identify the MHOs. PDRs have typical low flux ratios of ∼1.5–3, while the vast majority of MHOs display flux ratios typical of C-type shocks (∼6–20). A few MHOs exhibit flux ratios consistent with expected values for J-type shocks (∼3–4), but these are located in regions that may be contaminated with fluorescent emission. Some previously reported MHOs have low flux ratios, and are likely parts of PDRs rather than shocks indicative of outflows. We identify a total of 36 outflows across the 22 target regions where MHOs were detected. In over half these regions, MHO arrangements and fluorescent structures trace features present in CO outflow maps, suggesting that the CO emission traces a combination of dynamical effects, which may include gas entrained in expanding PDRs as well as bipolar outflows. Where possible, we link MHO complexes to distinct outflows and identify candidate driving sources.
Gravitational Waves from Stellar Black Hole Binaries and the Impact on Nearby Sun-like Stars
Authors: Lopes Ilídio , Silk Joseph 
Published: July 2017

Abstract
We investigate the impact of resonant gravitational waves on quadrupole acoustic modes of Sun-like stars located nearby stellar black hole binary systems (such as GW150914 and GW151226). We find that the stimulation of the low-overtone modes by gravitational radiation can lead to sizeable photometric amplitude variations, much larger than the predictions for amplitudes driven by turbulent convection, which in turn are consistent with the photometric amplitudes observed in most Sun-like stars. For accurate stellar evolution models, using up-to-date stellar physics, we predict photometric amplitude variations of 1–103 ppm for a solar mass star located at a distance between 1 au and 10 au from the black hole binary and belonging to the same multi-star system. The observation of such a phenomenon will be within the reach of the Plato mission because the telescope will observe several portions of the Milky Way, many of which are regions of high stellar density with a substantial mixed population of Sun-like stars and black hole binaries.
The Star Formation Histories of Disk Galaxies: The Live, the Dead, and the Undead
Authors: Oemler Augustus , Abramson Louis E. , Gladders Michael D. , Dressler Alan , Poggianti Bianca M. , Vulcani Benedetta 
Published: July 2017

Abstract
We reexamine the properties of local galaxy populations using published surveys of star formation, structure, and gas content. After recalibrating star formation measures, we are able to reliably measure specific star formation rates well below that of the so-called “main sequence” of star formation versus mass. We find an unexpectedly large population of quiescent galaxies with star formation rates intermediate between the main sequence and passive populations and with disproportionately high star formation rates. We demonstrate that a tight main sequence is a natural outcome of most histories of star formation and has little astrophysical significance but that the quiescent population requires additional astrophysics to explain its properties. Using a simple model for disk evolution based on the observed dependence of star formation on gas content in local galaxies, and assuming simple histories of cold gas inflow, we show that the evolution of galaxies away from the main sequence can be attributed to the depletion of gas due to star formation after a cutoff of gas inflow. The quiescent population is composed of galaxies in which the density of disk gas has fallen below a threshold for star formation probably set by disk stability. The evolution of galaxies beyond the quiescent state to gas exhaustion and the end of star formation requires another process, probably wind-driven mass loss. The environmental dependence of the three galaxy populations is consistent with recent numerical modeling, which indicates that cold gas inflows into galaxies are truncated at earlier epochs in denser environments.
Radiative Heating in the Kinetic Mode of AGN Feedback
Authors: Xie Fu-Guo , Yuan Feng , Ho Luis C. 
Published: July 2017

Abstract
AGN feedback is now widely believed to play a crucial role in the co-evolution between the central black hole and its host galaxy. Two feedback modes have been identified, namely the radiative and kinetic modes, which correspond to the luminous AGNs and low-luminosity AGNs (LLAGNs), respectively. In this paper, we investigate the radiative heating in the kinetic mode. This process is potentially important because (1) the radiation power of LLAGNs is higher than the jet power over a wide parameter range, (2) the spectral energy distribution of LLAGNs is such that the radiative heating is more effective compared to that of luminous AGNs with the same luminosity, and (3) most of the time in the lifecycle of an AGN is spent in the LLAGNs phase. In this paper, adopting the characteristic broadband spectral energy distributions of LLAGNs, we calculate the value of “Compton temperature” (

), which determines the radiative heating by Compton scattering. We find that

, depending on the spectrum of individual LLAGNs and at which distance from the black hole we evaluate the heating. We also compare this heating process with other radiative heating and cooling processes such as photoionization/recombination. Our result can be used for an accurate calculation of the radiative heating in the study of AGN feedback.
High-mass Starless Clumps in the Inner Galactic Plane: The Sample and Dust Properties
Authors: Yuan 袁敬 Jinghua 华 , Wu 吴月 Yuefang 芳 , Ellingsen Simon P. , II Neal J. Evans , Henkel Christian , Wang 王 Ke 科 , Liu 刘洪 Hong-Li 礼 , Liu 刘 Tie 铁 , Li 李金 Jin-Zeng 增 , Zavagno Annie 
Published: July 2017

Abstract
We report a sample of 463 high-mass starless clump (HMSC) candidates within

and

. This sample has been singled out from 10,861 ATLASGAL clumps. None of these sources are associated with any known star-forming activities collected in SIMBAD and young stellar objects identified using color-based criteria. We also make sure that the HMSC candidates have neither point sources at 24 and 70 μm nor strong extended emission at 24 μm. Most of the identified HMSCs are infrared dark, and some are even dark at 70 μm. Their distribution shows crowding in Galactic spiral arms and toward the Galactic center and some well-known star-forming complexes. Many HMSCs are associated with large-scale filaments. Some basic parameters were attained from column density and dust temperature maps constructed via fitting far-infrared and submillimeter continuum data to modified blackbodies. The HMSC candidates have sizes, masses, and densities similar to clumps associated with Class II methanol masers and H ii regions, suggesting that they will evolve into star-forming clumps. More than 90% of the HMSC candidates have densities above some proposed thresholds for forming high-mass stars. With dust temperatures and luminosity-to-mass ratios significantly lower than that for star-forming sources, the HMSC candidates are externally heated and genuinely at very early stages of high-mass star formation. Twenty sources with equivalent radii

pc and mass surface densities

g cm−2 could be possible high-mass starless cores. Further investigations toward these HMSCs would undoubtedly shed light on comprehensively understanding the birth of high-mass stars.
Resolving Orbital and Climate Keys of Earth and Extraterrestrial Environments with Dynamics (ROCKE-3D) 1.0: A General Circulation Model for Simulating the Climates of Rocky Planets
Authors: Way M. J. , Aleinov I. , Amundsen David S. , Chandler M. A. , Clune T. L. , Genio A. D. Del , Fujii Y. , Kelley M. , Kiang N. Y. , Sohl L. , Tsigaridis K. 
Published: July 2017

Abstract
Resolving Orbital and Climate Keys of Earth and Extraterrestrial Environments with Dynamics (ROCKE-3D) is a three-dimensional General Circulation Model (GCM) developed at the NASA Goddard Institute for Space Studies for the modeling of atmospheres of solar system and exoplanetary terrestrial planets. Its parent model, known as ModelE2, is used to simulate modern Earth and near-term paleo-Earth climates. ROCKE-3D is an ongoing effort to expand the capabilities of ModelE2 to handle a broader range of atmospheric conditions, including higher and lower atmospheric pressures, more diverse chemistries and compositions, larger and smaller planet radii and gravity, different rotation rates (from slower to more rapid than modern Earth’s, including synchronous rotation), diverse ocean and land distributions and topographies, and potential basic biosphere functions. The first aim of ROCKE-3D is to model planetary atmospheres on terrestrial worlds within the solar system such as paleo-Earth, modern and paleo-Mars, paleo-Venus, and Saturn’s moon Titan. By validating the model for a broad range of temperatures, pressures, and atmospheric constituents, we can then further expand its capabilities to those exoplanetary rocky worlds that have been discovered in the past, as well as those to be discovered in the future. We also discuss the current and near-future capabilities of ROCKE-3D as a community model for studying planetary and exoplanetary atmospheres.
L’échec d’un procès politique : Riom, 19 février-11 avril 1942
Authors: Jean Jean-Paul 
Published: July 2017

Dans un contexte de Seconde Guerre mondiale et des pleins pouvoirs conférés à Vichy, sans voies de recours, avec des entorses aux principes fondamentaux du droit et au détriment de l’indépendance de la justice a été instituée la Cour suprême de justice, du 30 juillet 1940 au 21 mai 1943, pour condamner les crimes de trahison. Le procès de Riom a ainsi répondu à une gestion politico-judiciaire qui donne à penser que les magistrats étaient aux ordres et Vichy sous la coupe des Allemands. Pourtant, Blum, Daladier et Gamelin ont été condamnés par le maréchal Pétain ! À la Libération, ce procès contre la République que voulait Vichy s’est retourné contre lui.