Published August 1999 | Version v1
Journal article

Evidence for Corotating Clouds in the Be Star ζ Tauri

  • 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