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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Published in | The Astrophysical journal Vol. 952; no. 2; pp. 102 - 120 |
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Main Authors | , , , , , , , |
Format | Journal Article |
Language | English |
Published |
Philadelphia
The American Astronomical Society
01.08.2023
IOP Publishing |
Subjects | |
Online Access | Get full text |
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