VizieR Online Data Catalog: Modelling of AGB stars in the LMC (Gullieuszik+, 2012)

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).