Powerful H 2 Line Cooling in Stephan’s Quintet. II. Group-wide Gas and Shock Modeling of the Warm H 2 and a Comparison with [C II] 157.7 μ m Emission and Kinematics - Observatoire de Paris
Journal Articles The Astrophysical Journal Year : 2017

Powerful H 2 Line Cooling in Stephan’s Quintet. II. Group-wide Gas and Shock Modeling of the Warm H 2 and a Comparison with [C II] 157.7 μ m Emission and Kinematics

P. Appleton
  • Function : Author
Infrared Processing and Analysis Center
P. Guillard
A. Togi
  • Function : Author
K. Alatalo
  • Function : Author
F. Boulanger
  • Function : Author
M. Cluver
  • Function : Author
G. Pineau Des Forêts
  • Function : Author
Institut d'astrophysique spatiale
Observatoire de Paris
U. Lisenfeld
Departamento Física Teórica y del Cosmos
P. Ogle
  • Function : Author
K. Xu
  • Function : Author

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Physics [physics] Astrophysics [astro-ph]

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https://hal-obspm.ccsd.cnrs.fr/obspm-02269971

Submitted on : Friday, August 23, 2019-2:49:37 PM

Last modification on : Thursday, June 13, 2024-4:20:04 PM

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obspm-02269971 , version 1 (23-08-2019)

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P. Appleton, P. Guillard, A. Togi, K. Alatalo, F. Boulanger, et al.. Powerful H 2 Line Cooling in Stephan’s Quintet. II. Group-wide Gas and Shock Modeling of the Warm H 2 and a Comparison with [C II] 157.7 μ m Emission and Kinematics. The Astrophysical Journal, 2017, 836 (1), pp.76. ⟨10.3847/1538-4357/836/1/76⟩. ⟨obspm-02269971⟩

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