Determination of Effective Temperatures and Luminosities for Rotating Stars

Details Determination of Effective Temperatures and Luminosities for Rotating Stars Determination of Effective Temperatures and Luminosities for Rotating Stars

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008apj...683..441g&link_type=abstract

The Astrophysical Journal, Volume 683, Issue 1, pp. 441-448.

Astronomy and Astrophysics

Astronomy

8

Stars: Atmospheres, Stars: Rotation

Scientific paper

Spectral energy distributions for models of arbitrarily rotating stars are computed using two-dimensional rotating stellar models, NLTE plane-parallel model atmospheres, and a code to integrate the appropriately weighted intensities over the visible surface of the stellar disk. The spectral energy distributions depend on the inclination angle between the observer and the rotation axis of the model. We use these curves to deduce what one would infer the model's luminosity and effective temperature to be assuming the object was nonrotating.

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