MC AGB & red supergiants lum. and dM/dt (Groenewegen+, 2009)

Details MC AGB & red supergiants lum. and dM/dt (Groenewegen+, 2009) MC AGB & red supergiants lum. and dM/dt (Groenewegen+, 2009)

Aug 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ycat..35061277g&link_type=abstract

VizieR On-line Data Catalog: J/A+A/506/1277. Originally published in: 2009A&A...506.1277G

Computer Science

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

Scientific paper

Dust radiative transfer models are presented for 101 carbon stars and 86 oxygen-rich evolved stars in the Magellanic Clouds for which 5-35um Spitzer IRS spectra are available. The spectra are complemented with available optical and infrared photometry to construct the spectral energy distribution. A minimisation procedure is used to fit luminosity, mass-loss rate and dust temperature at the inner radius. Different effective temperatures and dust content are also considered. Periods from the literature and from new OGLE-III data are compiled and derived.
(4 data files).

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