Published 1982
| Version v1
Book
The IUE observations of W UMa
Creators
- 1. Max-Planck-Institut fuer Physik und Astrophysik, Garching (Germany, F.R.). Inst. fuer Astrophysik
- 2. Cambridge Univ. (UK). Inst. of Astronomy
Description
The low resolution, phase averaged SWP spectra reveal the trend of increased transition-region line intensities for higher temperatures of ion formation which was previously observed for other active systems. Two series of low resolution LWR spectra covering two full orbital periods have been used to check the photometric results from the ANS satellite and a good agreement is found for the 2200 A band. Wavelength shifts and changes in the intensity of the blended Mg II emission feature are not inconsistent with the ANS result that the more massive component is the more active one in the W UMa system. (Auth.)
Additional details
Publishing Information
- Publisher
- D. Reidel.
- Imprint Place
- Dordrecht (Netherlands)
- ISBN
- 90-277-1436-3
- Imprint Title
- Binary and multiple stars as tracers of stellar evolution
- Imprint Pagination
- 531 p.
- Journal Volume
- 98
- Series
- Astrophysics and space science library.
- Journal Page Range
- p. 309-315.
Conference
- Title
- 69. Colloquium of the IAU on binary and multiple stars as tracers of stellar evolution.
- Dates
- 31 Aug - 3 Sep 1981.
- Place
- Bamberg (Germany, F.R.).
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- Netherlands
- INIS RN
- 14744535
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- BINARY STARS; EMISSION SPECTRA; MAGNESIUM IONS; ORBITS; ULTRAVIOLET SPECTRA; VARIATIONS
- Descriptors DEC
- ATOMIC IONS; CHARGED PARTICLES; IONS; SPECTRA; STARS
Optional Information
- Notes
- Imprint:Includes subject index.