ALMA Monitoring of Millimeter Line Variation in IRC +10216. I. Overview of Millimeter Variability
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ab3d37/pdf
Reference30 articles.
1. Physical conditions near red giant and supergiant stars - an interpretation of SiO VLBI maps
2. UNVEILING THE DUST NUCLEATION ZONE OF IRC+10216 WITH ALMA
3. DISCOVERY OF TIME VARIATION OF THE INTENSITY OF MOLECULAR LINES IN IRC+10216 IN THE SUBMILLIMETER AND FAR-INFRARED DOMAINS
4. VIBRATIONALLY EXCITED C 4 H
5. The abundance distribution of C4H in IRC + 10216
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3. Investigating Anomalous Photochemistry in the Inner Wind of IRC+10216 through Interferometric Observations of HC3N;The Astrophysical Journal;2022-12-01
4. Vibrationally excited HCN transitions in circumstellar envelopes of carbon-rich AGB stars;Astronomy & Astrophysics;2022-10
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