No CrossRef data available.
Article contents
Preliminary results on SiO v=3 J=1−0 maser emission from AGB stars
Published online by Cambridge University Press: 24 July 2012
Abstract
We present the results of SiO maser observations at 43 GHz toward two AGB stars using the VLBA. Our preliminary results on the relative positions of the different J=1–0 SiO masers (v=1,2 and 3) indicate that the current ideas on SiO maser pumping could be wrong at some fundamental level. A deep revision of the SiO pumping models could be necessary.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 8 , Symposium S287: Cosmic Masers - from OH to H0 , January 2012 , pp. 252 - 253
- Copyright
- Copyright © International Astronomical Union 2012