No CrossRef data available.
Article contents
HCN (J=1-0) maser emission in the bright carbon star Y CVn
Published online by Cambridge University Press: 03 August 2017
Abstract
We present high resolution observations of HCN(J=1-0) line in the bright carbon star Y CVn. With an angular resolution of 0.5 arcsec we are able to resolve the HCN envelope around Y CVn. The HCN(J=1-0) line profile toward the central position exhibits several strong spikes having brightness temperature in excess of 1000 K. This result indicates that the J=1-0 line is masing. We also discuss the pump mechanism of this maser and the implication for the determination of the HCN abundance.
- Type
- Part 2. Stellar Masers
- Information
- Symposium - International Astronomical Union , Volume 206: Cosmic Masers: From Protostars to Blackholes , 2002 , pp. 340 - 342
- Copyright
- Copyright © Astronomical Society of the Pacific 2002