Maser emission of SiO isotopes from stars and the pumping mechanism

Details Maser emission of SiO isotopes from stars and the pumping mechanism Maser emission of SiO isotopes from stars and the pumping mechanism

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989cha%26a..13...46z&link_type=abstract

Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 13, March 1989, p. 46-51. Translation.

Astronomy and Astrophysics

Astrophysics

Interstellar Masers, Molecular Clouds, Silicon Isotopes, Silicon Oxides, Stellar Radiation, Orion Constellation, Red Giant Stars, Stellar Envelopes, Supergiant Stars

Scientific paper

The detection of (Si-29)O v = 0, J = 1-0 maser from VY CMa, VX Sgr, and
U Her, is reported. In addition, the (Si-30)O maser has been detected
from VY CMa. It is shown that the (Si-29)O aand (Si-30)O masers are
pumped by molecular collision and stellar IR radiation.

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