Far-ultraviolet observations of BW Vulpeculae with Voyager 2

Details Far-ultraviolet observations of BW Vulpeculae with Voyager 2 Far-ultraviolet observations of BW Vulpeculae with Voyager 2

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...281..766b&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 281, June 15, 1984, p. 766-773.

Other

15

Light Curve, Stellar Luminosity, Stellar Spectrophotometry, Stellar Temperature, Ultraviolet Spectra, Variable Stars, Iue, Ultraviolet Spectroscopy, Voyager 2 Spacecraft

Scientific paper

BW Vul has been the subject of numerous ground-based spectroscopic and photometric studies. However, observations in the ultraviolet have been limited. The Voyager 2 observations presented in the current study include the first observations of BW Vul shortward of 1200 A. Voyager 2 observations in the 912-1700 A region are employed to investigate the variations in the temperature, radius, and luminosity of BW Vul during a pulsation cycle. Attention is given to details regarding the observations, the light curves representing the variation of BW Vul at effective wavelengths of 1050 A and 1395 A, the UV spectra, comparisons with other stars, comparisons with models, and the amplitude-wavelength relation.

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