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Interstellar clouds containing optically thin H2

Jura, M.·1975·The Astrophysical Journal

Abstract

The theory of Black and Delgarno that the relative populations of the excited rotational levels of H2 can be understood in terms of cascading following absorption in the Lyman and Werner bands is employed to infer the gas densities and radiation fields within diffuse interstellar clouds containing H2 that is optically thin in those bands. The procedure is described for computing the populations of the different rotation levels, the relative distribution among the different rotation levels of newly formed H2 is determined on the basis of five simplified models, and the rate of H2 formation is estimated. The results are applied to delta Ori, two components of iota Ori, the second components of rho Leo and zeta Ori, tau Sco, gamma Vel, and zeta Pup. The inferred parameters are summarized for each cloud.

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Metadata

Authors
Jura, M.
Venue
The Astrophysical Journal
Published
1975-05
Volume
197
Pages
575
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2249042401
Cited by
192
References
0
FWCI
4.51
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Interstellar clouds containing optically thin H2. https://app.cochat.ai/papers/10.1086/153545
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Jura, M. (1975). Interstellar clouds containing optically thin H2. The Astrophysical Journal. https://doi.org/10.1086/153545

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