Structure of the W3A Low-density Foreground Region

We present analysis of [O i ] 63 μ m and CO J = 5 − 4 and 8 − 7 multiposition data in the W3A region and use it to develop a model for the extended low-density foreground gas that produces absorption features in the [O i ] and J = 5 − 4 CO lines. We employ the extinction to the exciting stars of the...

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Bibliographic Details
Published inThe Astrophysical journal Vol. 952; no. 2; pp. 102 - 120
Main Authors Goldsmith, Paul. F., Langer, William D., Seo, Youngmin, Pineda, Jorge, Stutzki, Jürgen, Guevara, Christian, Aladro, Rebeca, Justen, Matthias
Format Journal Article
LanguageEnglish
Published Philadelphia The American Astronomical Society 01.08.2023
IOP Publishing
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