Using UV spectra obtained with FUSE, HST, and/or IUE, we determine interstellar column densities of 12CO, 13CO, and/or C₂ for ten Galactic sight lines with 0. 37

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Abundances and Behavior of 12 CO, 13 CO, and C 2 in Translucent Sight Lines | Synapse

Cite This Study

Sonnentrucker et al. (Mon,) studied this question.

synapsesocial.com/papers/6a1d6762b1a9bd2ac02f1f86 https://doi.org/https://doi.org/10.1086/508687

Also Consider

Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context:

1The CO-12/CO-13 abundance ratio toward Zeta Ophiuchi1982 · 36 citations
2The Photodissociation and Chemistry of Interstellar CO: Erratum1990 · 6 citations
3Chemical transitions for interstellar C2 and CN in cloud envelopes1994 · 126 citations
4Ultra-high-resolution observations of the intrinsic line profiles of interstellar CH, CH+ and CN1995 · 66 citations
5Molecular Gas in Galaxies1991 · 581 citations

Also Consider

Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context:

1The CO-12/CO-13 abundance ratio toward Zeta Ophiuchi1982 · 36 citations
2The Photodissociation and Chemistry of Interstellar CO: Erratum1990 · 6 citations
3Chemical transitions for interstellar C2 and CN in cloud envelopes1994 · 126 citations
4Ultra-high-resolution observations of the intrinsic line profiles of interstellar CH, CH+ and CN1995 · 66 citations
5Molecular Gas in Galaxies1991 · 581 citations