Published October 1990 | Version v1
Journal article

Atmospheric parameters of the white-dwarf companion to HD 74389

  • 1. Steward Observatory, Tucson, AZ (USA)

Description

An optical slit spectrum of the recently discovered DA white-dwarf companion to the A2 V star HD 74389 is presented. Fits of theoretical spectra to six observed Balmer lines lead to estimates of Tc = 41,000 (+4000, -1000) K and log g = 7.85 (+0.20, -0.06). The latter implies that the white dwarf does not have a substantially higher mass than the mean for field DA white dwarfs. These parameters lead to an estimated M(v) = +9.4, a value not inconsistent with the assumption that the two stars lie at a similar distance from the sun. 10 refs

Additional details

Publishing Information

Journal Title
Publications of the Astronomical Society of the Pacific
Journal Volume
102
Series
Publ. Astron. Soc. Pac.
Journal Page Range
1126-1130
ISSN
0004-6280
CODEN
PASPA

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
22032957
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
BALMER LINES; BINARY STARS; CHARGE-COUPLED DEVICES; DISTANCE; MASS; STELLAR ATMOSPHERES; VISIBLE SPECTRA; WHITE DWARF STARS
Descriptors DEC
ATMOSPHERES; DWARF STARS; SEMICONDUCTOR DEVICES; SPECTRA; STARS