The spectroscopic orbits and physical parameters of GG Car

Details The spectroscopic orbits and physical parameters of GG Car The spectroscopic orbits and physical parameters of GG Car

Jul 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..272..523m&link_type=abstract

Active OB stars: structure, evolution, mass loss, and critical limits, Proceedings of the International Astronomical Union, IAU

Astronomy and Astrophysics

Astronomy

Stars: Individual (Gg Car), Stars: Emission-Line, Stars: Fundamental Parameters

Scientific paper

GG Car is a peculiar B type star with emission lines classified as a B[e] supergiant star. In this work we present a spectral analysis of this system based on spectra obtained at Casleo. We fit the spectral energy distribution adopting a model for the gas and dust circumstellar components and thus we obtain the physical parameters of the star and its environment.

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