Correlation of R Cassiopeia's SiO Maser Properties

Details Correlation of R Cassiopeia's SiO Maser Properties Correlation of R Cassiopeia's SiO Maser Properties

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...20913704h&link_type=abstract

2007 AAS/AAPT Joint Meeting, American Astronomical Society Meeting 209, #137.04; Bulletin of the American Astronomical Society,

Astronomy and Astrophysics

Astronomy

Scientific paper

Silicon monoxide masers originate in the circumstellar environment of many long period variable stars. SiO emission from R Cassiopeia has been observed over several stellar periods in the v = 0, 1, 2, and 3, J=1-0 transitions. The integrated intensities have been analyzed for correlations. Since the masers are observed to occur at different distances from the star, the correlations constrain the possible pumping mechanisms.

Affiliated with

Also associated with

No associations

Rating

Correlation of R Cassiopeia's SiO Maser Properties 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 Correlation of R Cassiopeia's SiO Maser Properties, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Correlation of R Cassiopeia's SiO Maser Properties will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1161349