Photocentric and Photometric Variability of Red Supergiant Stars

Details Photocentric and Photometric Variability of Red Supergiant Stars Photocentric and Photometric Variability of Red Supergiant Stars

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aspc..445..169c&link_type=abstract

Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants. Proceedings of a conference held at University Ca

Astronomy and Astrophysics

Astronomy

Scientific paper

Red supergiant stars are characterized by large convection-related surface structures that cause surface inhomogeneities and shock waves. We explore the impact of granulation on photocentric and photometric variability using 3D simulations of convection with Co5BOLD and the post-processing radiative transfer code OPTIM 3D to compute spectra and intensity maps in the Gaia G band (325 - 1030 nm).

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