Infrared Detection of Abundant CS in the Hot Core AFGL 2591 at High Spectral Resolution with SOFIA/EXES-Reference-Cited by-同舟云学术

Infrared Detection of Abundant CS in the Hot Core AFGL 2591 at High Spectral Resolution with SOFIA/EXES

Published:2018-11-12 Issue:1 Volume:868 Page:L2
ISSN:2041-8213
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Barr Andrew G.^ORCID,Boogert Adwin,DeWitt Curtis N.,Montiel Edward,Richter Matthew J.^ORCID,Indriolo Nick^ORCID,Neufeld David A.^ORCID,Pendleton Yvonne,Chiar Jean,Dungee Ryan^ORCID,M. Tielens Alexander G. G.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/2041-8213/aaeb23/pdf

Reference50 articles.

1. The high-velocity molecular flows near young stellar objects

2. Energetic radiation and the sulfur chemistry of protostellar envelopes: submillimeter interferometry of AFGL 2591

3. Molecular abundances in OMC-1 - The chemical composition of interstellar molecular clouds and the influence of massive star formation

4. Highly Abundant HCN in the Inner Hot Envelope of GL 2591: Probing the Birth of a Hot Core?

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