Analysis of Fiege 66, another extremely silicon-deficient OB subdwarf

Details Analysis of Fiege 66, another extremely silicon-deficient OB subdwarf Analysis of Fiege 66, another extremely silicon-deficient OB subdwarf

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982esasp.176..309b&link_type=abstract

In ESA 3rd European IUE Conf. p 309-311 (SEE N83-11889 02-88)

Computer Science

Abundance, Silicon, Subdwarf Stars, Atmospheric Models, Chemical Composition, Iue, Stellar Gravitation, Stellar Temperature, Ultraviolet Spectroscopy

Scientific paper

A high resolution IUE spectrum from 1160 to 3230 A of Feige 66 was
analyzed by model atmosphere techniques differentially to OB subdwarf HD
149382. The stars have similar effective temperatures and surface
gravities, and exhibit remarkably similar abundance patterns.

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