ISO spectroscopy of AGB stars in the LMC

Details ISO spectroscopy of AGB stars in the LMC ISO spectroscopy of AGB stars in the LMC

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000esasp.456..161t&link_type=abstract

ISO beyond the peaks: The 2nd ISO workshop on analytical spectroscopy. Eds. A. Salama, M.F.Kessler, K. Leech & B. Schulz. ESA-SP

Physics

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

Scientific paper

In this paper we discuss ISO spectrophotometry of a sample of Asymptotic Giant Branch stars and Red Supergiants in the LMC. The observations were fitted with spectral energy distributions calculated using a radiative transfer code. In this way luminosities and mass loss rates for the stars as well as the chemical nature of the dust shells around the stars could be established. The luminosity and mass loss distributions of these stars are presented. We find clear luminosity distinctions between optical C-stars, dust enschrouded C-stars and M-type stars.

Affiliated with

Also associated with

No associations

Rating

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

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1610416