Probing the dust formation region in IRC +10216 with the high vibrational states of hydrogen cyanide
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361/201116717/pdf
Reference30 articles.
1. Agúndez, M. 2009, Ph.D., Universidad Autónoma de Madrid
2. Submillimeter molecular line observations of IRC +10216: Searches for MgH, SiH2, and HCO(+), and detection of hot HCN
3. Submillimeter‐ and Millimeter‐Wavelength Observations of SiO and HCN in Circumstellar Envelopes of AGB Stars
4. Cernicharo, J. 1985, ATM a code to compute atmospheric opacity up to 1 THz, IRAM internal report
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