Modelisation of AGB stars in the LMC (Gullieuszik+, 2012)

Details Modelisation of AGB stars in the LMC (Gullieuszik+, 2012) Modelisation of AGB stars in the LMC (Gullieuszik+, 2012)

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..35379105g&link_type=abstract

VizieR On-line Data Catalog: J/A+A/537/A105. Originally published in: 2012A&A...537A.105G

Physics

Magellanic Clouds, Stars: Giant, Stars: Carbon, Mass Loss

Scientific paper

Dust radiative transfer models are presented for 374 AGB star candidates in the VMC tile 83. The photometric spectral energy distribution is fitted using dust radiative transfer models. A minimisation procedure is used to fit the luminosity and optical depth of the dusty shell, which is then used to calculate the mass-loss rate. We also list the optical to mid-IR photometry for all 367 stars classified as AGB stars, and the reduced {chi} squared for best-fitting O- and C-rich models which were used to classify AGB stars.
(2 data files).

Affiliated with

Also associated with

No associations

Rating

Modelisation of AGB stars in the LMC (Gullieuszik+, 2012) 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 Modelisation of AGB stars in the LMC (Gullieuszik+, 2012), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Modelisation of AGB stars in the LMC (Gullieuszik+, 2012) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1676010