Theoretical and Observed Energy Distribution of Metal-Poor Stars

Details Theoretical and Observed Energy Distribution of Metal-Poor Stars Theoretical and Observed Energy Distribution of Metal-Poor Stars

Nov 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998larm.confe..98e&link_type=abstract

"IX Latin American Regional IAU Meeting, "Focal Points in Latin American Astronomy", held in Tonantzintla, Mexico, Nov 9-13, 199

Astronomy and Astrophysics

Astronomy

Scientific paper

We present a comparison between theoretical and observed energy distributions of a small sample of metal defficient A-K stars. Such comparison is intended to investigate the adequacy of current up to date Kurucz model atmospheres with different convection treatments. The stellar sample includes stars with [Fe/H] < -2.0 in the catalogue of high resolution [Fe/H] determinations of Cayrel et al. (1997). The Observed stellar spectra were collected at the Guillermo Haro Observatory covering the spectral interval 3800-7100 angstroms. In this poster paper we present preliminary results.

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