High sensitivity SiO maser survey for Mira variables

Details High sensitivity SiO maser survey for Mira variables High sensitivity SiO maser survey for Mira variables

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.118..237c&link_type=abstract

(IAU, Asian-Pacific Regional Meeting, 3rd, Kyoto, Japan, Sept. 30-Oct. 5, 1984) Astrophysics and Space Science (ISSN 0004-640X),

Astronomy and Astrophysics

Astrophysics

9

Emission Spectra, Interstellar Masers, Late Stars, Mira Variables, Silicon Oxides, Variable Stars, Spectral Sensitivity

Scientific paper

Simultaneous observations of the six transitions of SiO for 106 late-type stars were made. The SiO maser emission was detected in 83 stars. The υ = 3 maser emission was detected in eight stars, and the 29SiO υ = 0 emission in six stars. The 29SiO υ = 0 emission is stronger and narrower than that of 28SiO, suggesting that the 29SiO emission is masing.

Affiliated with

Also associated with

No associations

Rating

High sensitivity SiO maser survey for Mira variables does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with High sensitivity SiO maser survey for Mira variables, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High sensitivity SiO maser survey for Mira variables will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1844116