(1) The origin of the [CII]-deficit in a simulated dwarf galaxies starburst
Thomas G. Bisbas+ ApJ(2) Infrared Spectroscopy of free-floating planet candidates in Upper Scorpius and Ophiuchus
H. Bouy+ AAp 664, A111
(3) Collisional Charging in the Low Pressure Range of Protoplanetary Disks
T. Becker+ MNRAS(4) HCN snowlines in protoplanetary disks: constraints from ice desorption experiments
Jennifer B. Bergner+ ApJ(5) Transit Hunt for Young and Maturing Exoplanets (THYME) VIII: a Pleiades-age association harboring
two transiting planetary systems from Kepler, Madyson G. Barber+ AJ(6) A new phase of massive star formation? A luminous outflow cavity centred on an infrared quiet core
L. Bonne,+ AAp(7) Resolving desorption of complex organic molecules in a hot core: Transition from non-thermal
to thermal desorption or two-step thermal desorption? Laura A. Busch+AAp

(1) The origin of the [CII]-deficit in a simulated dwarf galaxies starburst
Thomas G. Bisbas+ ApJ

The [Cii]/FIR luminosity ratio is observed to decrease with increasing infrared luminosity.
The origin of the so called ʻ[Cii]-deficitʼ is still being investigated(1) optically thick [Cii] emission in large columns of dust,(2) conversion of singly (C+) to doubly (C2+) ionized carbon,(3) and fine-structure lines (e.g. [Oi]) overcoming [Cii] as coolantsMg=2x10^10M8
初期距離 5kpc
最近接距離1.46kpc
ΔMSPH=4M8[CII]

observation

simulation

FIRTg

Infrared Spectroscopy of free-floating planet candidates in Upper Scorpius and Ophiuchus
H. Bouy+ AAp 664, A111

H-band

Almendros-Abad+2022 Hcont

Low g

Field
Mid g

TLI-g(λ1.5-1.565H2Oband)
Mid gAllers & Liu 2013

FFP candidateのHcont index

Field

TLI-g index

Low g

F1.56-1.58μ/F1.625-1.635μ<latexit sha1_base64="P8qauftXqOvsnzrIUGcUooezetY=">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</latexit>Hcont =Fcont
Fline 1.56μ1.67μFline Fcont
1.47<latexit sha1_base64="QxAQ52I75ronrWf9eoz83FuGp7s=">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</latexit><latexit sha1_base64="9M3O0kW5ARjWPrJvrOZSOIpOuXo=">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</latexit>

全17個

16個
若い低温度星L型スペクトル
M=0.004-0.013M8

1個
contamination

1Myr

10Myr

(3) Collisional Charging in the Low Pressure Range of Protoplanetary Disks
T. Becker+ MNRAS

絶縁破壊電圧

直径1mmガラス球をフラスコに衝突させ、帯電量を図る実験

388K

似ている

(4) HCN snowlines in protoplanetary disks: constraints from ice desorption experimentsJennifer B. Bergner+ ApJ

(5) Transit Hunt for Young and Maturing Exoplanets (THYME) VIII: a Pleiades-age association harboring
two transiting planetary systems from Kepler, Madyson G. Barber+ AJ

(6) A new phase of massive star formation? A luminous outflow cavity centred on an infrared quiet core
L. Bonne,+ AAp(1) Hub filament structure(2) Two warm regions
N1,N2
fragmentのH1の両側に70μ bipolar nebulosity
S106, RCW36でも⾒える
この天体では原始星に相当する⾚外線源がない
NHI

F70μNHITd

SED

12<latexit sha1_base64="1Sb5k43LLmHKJoJ5pOce7p8y3lQ=">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</latexit>

2.3 ⇥ 103 L<latexit sha1_base64="6Bsh9+63FlS5U/xKExnpgEprKX4=">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</latexit>

ほぼ同⼀51+29327 L
2.1 ⇥ 10 L
nebulosity
fragment

CO(21) total intensity<latexit sha1_base64="7HtqBG/37hp0BfEEqAWlkVcUVig=">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</latexit><latexit sha1_base64="yQzYT40q4i4mgo14hAcsrI3cZp0=">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</latexit>

開⼝⾓105度

0.66pcH4

全光度

4.4 ⇥ 103 L<latexit sha1_base64="3fY4atvKJ1YqkerClqGkrtaAYvQ=">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</latexit>

bipolar nebulosityóbipolar outflow? (high velocity wing)
仮定 ✓incl = 57.6
<latexit sha1_base64="8r+KGjDaZHtQJQytHL0c/fSFwrg=">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</latexit><latexit sha1_base64="Ilh+Hxr2GEdwqQg7h3QKTlU2yDM=">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</latexit>

⾚⻘対称に運動量を放出

dM V= 2.8 ⇥ 10 3 M km s 1 yr 1dt

⼤質量星形成初期の値と等しい

H10.55pc

開⼝⾓72度プランマー型コア
アウトフローキャビティ

アウトフローキャビティ

2つのピークが両側にできるか？

パッシブフレア円盤

(7) Resolving desorption of complex organic molecules in a hot core: Transition from non-thermal
to thermal desorption or two-step thermal desorption? Laura A. Busch+AAp