Ultraviolet analysis of the peculiar F supergiant HD 112374

Details Ultraviolet analysis of the peculiar F supergiant HD 112374 Ultraviolet analysis of the peculiar F supergiant HD 112374

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984nascp2349..352b&link_type=abstract

In NASA. Goddard Space Flight Center Future of Ultraviolet Astronomy Based on Six Years of IUE Res. p 352-354 (SEE N85-20961 1

Astronomy and Astrophysics

Astronomy

Cepheid Variables, Energy Distribution, F Stars, Iue, Supergiant Stars, Ultraviolet Spectra, Flux (Rate), Ultraviolet Astronomy, Variable Stars

Scientific paper

The authors have studied the ultraviolet energy distribution of the metal-poor supergiant HD 112347. They need a temperature Teff = 5500±100K, log g = -0.3±0.3 and a metal deficiency of log Z/Z_sun; = -0.7 in order to find agreement between theoretical and observed ultraviolet energy distributions with a reddening of E(B-V) ≤ 0.1 consistent with its galactic latitude of +36°.

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