Simultaneous observations of maser lines of 28SiO in evolved stars

Details Simultaneous observations of maser lines of 28SiO in evolved stars Simultaneous observations of maser lines of 28SiO in evolved stars

Jan 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26a...329..219p&link_type=abstract

Astronomy and Astrophysics, v.329, p.219-228 (1998)

Astronomy and Astrophysics

Astrophysics

15

Stars: Agb, Post-Agb, Masers, Stars: Circumstellar Matter, Radio-Lines: Stars

Scientific paper

We present simultaneous observations of several rotational lines of (28) SiO in the v=1, 2, 3, and 4 vibrationally excited states toward O-rich evolved stars. All the data were taken in a relatively short period of 65 days, which allows a comparative study of the (28) SiO maser lines intensities and profiles. The observed differences concerning intensity and line shape among the different maser lines suggest that infrared overlaps deeply affect the pumping of some SiO masers. We qualitatively discuss this effect with consideration to the IR overlaps at 8 mu m between the various SiO isotopomers and between (28) SiO and water vapor
Tables 5 to 16 are only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/Abstract.html.

Affiliated with

Also associated with

No associations

Rating

Simultaneous observations of maser lines of 28SiO in evolved stars 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 Simultaneous observations of maser lines of 28SiO in evolved stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Simultaneous observations of maser lines of 28SiO in evolved stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1650335