Energetic radiation and the sulfur chemistry of protostellar envelopes: submillimeter interferometry of AFGL 2591
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20078032/pdf
Reference33 articles.
1. Highly Abundant HCN in the Inner Hot Envelope of GL 2591: Probing the Birth of a Hot Core?
2. An X-Ray Survey of Very Young Stellar Objects
3. Observation of Infrared and Radio Lines of Molecules toward GL 2591 and Comparison to Physical and Chemical Models
4. Sulfuretted Molecules in Hot Cores
5. A laboratory survey of the thermal desorption of astrophysically relevant molecules
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1. Disk fragmentation in high-mass star formation;Astronomy & Astrophysics;2021-11
2. Multiwavelength modelling of the circumstellar environment of the massive protostar AFGL 2591 VLA 3;Monthly Notices of the Royal Astronomical Society;2020-09-08
3. Chemical complexity in high-mass star formation;Astronomy & Astrophysics;2019-11
4. Infrared Detection of Abundant CS in the Hot Core AFGL 2591 at High Spectral Resolution with SOFIA/EXES;The Astrophysical Journal;2018-11-12
5. Approaching hell’s kitchen: Molecular daredevil clouds in the vicinity of Sagittarius A*;Astronomy & Astrophysics;2017-07
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