The Circumstellar Shell of the Post-AGB Star IRAS 22272+5435

Details The Circumstellar Shell of the Post-AGB Star IRAS 22272+5435 The Circumstellar Shell of the Post-AGB Star IRAS 22272+5435

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..378..339s&link_type=abstract

Why Galaxies Care About AGB Stars: Their Importance as Actors and Probes. ASP Conference Series, Vol. 378, proceedings of the co

Astronomy and Astrophysics

Astronomy

Scientific paper

We have analysed optical spectra of the carbon-rich post-AGB star IRAS 22272+5435. The circumstellar components of molecular lines of CN (Red System) and C2 (Phillips and Swan bands) were identified and measured. The mechanism of excitation of the rotational levels of the ground electronic states of CN and C2 was analysed with a non-LTE code. An empirical model accounting for the observed spectral energy distribution was used as the physical model of the shell. An extensive chemical model was constructed based on the elemental abundances obtained from the analysis of optical atomic lines.

Affiliated with

Also associated with

No associations

Rating

The Circumstellar Shell of the Post-AGB Star IRAS 22272+5435 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 The Circumstellar Shell of the Post-AGB Star IRAS 22272+5435, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Circumstellar Shell of the Post-AGB Star IRAS 22272+5435 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-736004