Near-infrared spectroscopy of post-AGB stars.

Details Near-infrared spectroscopy of post-AGB stars. Near-infrared spectroscopy of post-AGB stars.

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26a...299...69o&link_type=abstract

Astronomy and Astrophysics, v.299, p.69

Astronomy and Astrophysics

Astrophysics

27

Stars: Circumstellar Matter, Stars: Evolution, Stars: Mass Loss, Stars: Agb And Post-Agb

Scientific paper

The results of a medium resolution near-infrared spectral survey of 18 post-AGB candidate stars are presented. Most of the stars have near-infrared hydrogen lines in absorption, which is normal for their spectral types. Three stars, HD 101584, HD 179821 and HD 170756 have the CO first overtone bands in emission; in two of these the emission is variable. It is suggested that the CO emission is the result of post-AGB mass loss. HD 52961 shows the rarely occurring 3.5μm emission feature and is only the fourth object in which this feature has been detected.

Affiliated with

Also associated with

No associations

Rating

Near-infrared spectroscopy of post-AGB 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 Near-infrared spectroscopy of post-AGB stars., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Near-infrared spectroscopy of post-AGB stars. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1168296