Published August 1999
| Version v1
Journal article
Evidence for Corotating Clouds in the Be Star ζ Tauri
Creators
- 1. South African Astronomical Observatory, PO Box 9, Observatory 7935, West Cape (South Africa)
- 2. Applied Theoretical and Computational Physics Division, Los Alamos National Laboratory, X-TA, MS B-220, Los Alamos, NM 87545 (United States)
Description
We reexamine a time series of spectroscopic data of the Be star ζ Tauri obtained by Kaye and Gies. When the difference spectra are folded with the 0.777 day period, a distinctive pattern emerges. This pattern is not the standard barber pole diagram expected from nonradial pulsation but is instead a pattern of two sinusoidal variations of enhanced absorption having different amplitudes. We interpret these results as additional evidence for corotating clouds, recently suggested as an explanation of the variations observed in several other Be stars and as indirect evidence for the possible presence of magnetic fields. copyright copyright 1999. The American Astronomical Society
Additional details
Publishing Information
- Journal Title
- Astrophysical Journal
- Journal Volume
- 521
- Journal Issue
- 1
- Journal Page Range
- p. 407-413
- ISSN
- 0004-637X
- CODEN
- ASJOAB
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 31001486
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- EMISSION SPECTRA; LINE WIDTHS; MAGNETIC FIELDS; STARS; STELLAR ATMOSPHERES; VISIBLE SPECTRA
- Descriptors DEC
- ATMOSPHERES; SPECTRA