Distance and mass of pulsating stars from multicolour photometry and atmospheric models

Details Distance and mass of pulsating stars from multicolour photometry and atmospheric models Distance and mass of pulsating stars from multicolour photometry and atmospheric models

2003-04-10

arxiv.org/abs/astro-ph/0304188v1

Astron.Astrophys. 403 (2003) 683

Astronomy and Astrophysics

Astrophysics

9 pages, 4 figures, 4 tables. Accepted in Astronomy and Astrophysics

Scientific paper

10.1051/0004-6361:20030410

For determining distance and mass of pulsating stars a new, purely
photometric method is described in which radial velocity observations are not
needed. The method is compared with the Baade-Wesselink method. As an example
the RR Lyrae variable SU Dra is given.

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