The Origin of [C ii] 158 μm Emission toward the H ii Region Complex S235

L. D. Anderson, Z. Makai, M. Luisi, M. Andersen, D. Russeil, M. R. Samal, N. Schneider, P. Tremblin, A. Zavagno, M. S. Kirsanova, V. Ossenkopf-Okada, A. M. Sobolev

Результат исследований: Вклад в журналСтатья

Язык оригиналаАнглийский
Номер статьи11
Число страниц18
ЖурналAstrophysical Journal
Том882
Номер выпуска1
DOI
СостояниеОпубликовано - 1 сен 2019

Отпечаток

hydrogen
Wide-field Infrared Survey Explorer
tracers
tracer
star formation
gas
SOFIA (airborne observatory)
radio
galaxies
radio telescopes
spectroscopic analysis
ultraviolet radiation
molecular gases
tracing
gases
complement
radiation distribution
recombination
continuums
analysis

Предметные области ASJC Scopus

  • Astronomy and Astrophysics
  • Space and Planetary Science

Предметные области WoS

  • Астрономия и астрофизика

Цитировать

Anderson, L. D., Makai, Z., Luisi, M., Andersen, M., Russeil, D., Samal, M. R., ... Sobolev, A. M. (2019). The Origin of [C ii] 158 μm Emission toward the H ii Region Complex S235. Astrophysical Journal, 882(1), [11]. https://doi.org/10.3847/1538-4357/ab1c59
Anderson, L. D. ; Makai, Z. ; Luisi, M. ; Andersen, M. ; Russeil, D. ; Samal, M. R. ; Schneider, N. ; Tremblin, P. ; Zavagno, A. ; Kirsanova, M. S. ; Ossenkopf-Okada, V. ; Sobolev, A. M. / The Origin of [C ii] 158 μm Emission toward the H ii Region Complex S235. В: Astrophysical Journal. 2019 ; Том 882, № 1.
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title = "The Origin of [C ii] 158 μm Emission toward the H ii Region Complex S235",
keywords = "H II regions, infrared: ISM, radio continuum: ISM, techniques: photometric, DUST DYNAMICS, CII, MICRON, STAR-FORMATION, MULTIWAVELENGTH, EVOLUTION, SPECTROSCOPY, RADIO RECOMBINATION LINES, GALAXIES, HII-REGIONS",
author = "Anderson, {L. D.} and Z. Makai and M. Luisi and M. Andersen and D. Russeil and Samal, {M. R.} and N. Schneider and P. Tremblin and A. Zavagno and Kirsanova, {M. S.} and V. Ossenkopf-Okada and Sobolev, {A. M.}",
year = "2019",
month = "9",
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language = "English",
volume = "882",
journal = "Astrophysical Journal",
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Anderson, LD, Makai, Z, Luisi, M, Andersen, M, Russeil, D, Samal, MR, Schneider, N, Tremblin, P, Zavagno, A, Kirsanova, MS, Ossenkopf-Okada, V & Sobolev, AM 2019, 'The Origin of [C ii] 158 μm Emission toward the H ii Region Complex S235', Astrophysical Journal, том. 882, № 1, 11. https://doi.org/10.3847/1538-4357/ab1c59

The Origin of [C ii] 158 μm Emission toward the H ii Region Complex S235. / Anderson, L. D.; Makai, Z.; Luisi, M.; Andersen, M.; Russeil, D.; Samal, M. R.; Schneider, N.; Tremblin, P.; Zavagno, A.; Kirsanova, M. S.; Ossenkopf-Okada, V.; Sobolev, A. M.

В: Astrophysical Journal, Том 882, № 1, 11, 01.09.2019.

Результат исследований: Вклад в журналСтатья

TY - JOUR

T1 - The Origin of [C ii] 158 μm Emission toward the H ii Region Complex S235

AU - Anderson, L. D.

AU - Makai, Z.

AU - Luisi, M.

AU - Andersen, M.

AU - Russeil, D.

AU - Samal, M. R.

AU - Schneider, N.

AU - Tremblin, P.

AU - Zavagno, A.

AU - Kirsanova, M. S.

AU - Ossenkopf-Okada, V.

AU - Sobolev, A. M.

PY - 2019/9/1

Y1 - 2019/9/1

KW - H II regions

KW - infrared: ISM

KW - radio continuum: ISM

KW - techniques: photometric

KW - DUST DYNAMICS

KW - CII

KW - MICRON

KW - STAR-FORMATION

KW - MULTIWAVELENGTH

KW - EVOLUTION

KW - SPECTROSCOPY

KW - RADIO RECOMBINATION LINES

KW - GALAXIES

KW - HII-REGIONS

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U2 - 10.3847/1538-4357/ab1c59

DO - 10.3847/1538-4357/ab1c59

M3 - Article

AN - SCOPUS:85072335364

VL - 882

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 1

M1 - 11

ER -

Anderson LD, Makai Z, Luisi M, Andersen M, Russeil D, Samal MR и соавт. The Origin of [C ii] 158 μm Emission toward the H ii Region Complex S235. Astrophysical Journal. 2019 Сент. 1;882(1). 11. https://doi.org/10.3847/1538-4357/ab1c59