Published June 1988 | Version v1
Report Metadata-only

HD 207739 and other F + Be variables

Creators

  • 1. Space Telescope Science Inst., Baltimore, MD (USA)
  • 2. Toledo Univ., OH (USA). Dept. of Physics and Astronomy

Description

Various characteristics are compared and summarized for a group of composite spectrum stars which have strong H alpha emission and peculiar satellite UV spectra. Spectroscopic periods and photometric variability are now defined for most of these systems. Compared with normal non-interacting composite spectrum binaries, they exhibit excess flux in the middle UV region. This is believed to indicate the presence of an accretion disk

Part of:
A decade of UV astronomy with the IUE satellite. Volume 1

Additional details

Publishing Information

Imprint Title
A decade of UV astronomy with the IUE satellite. Volume 1
Imprint Pagination
448 p.
Journal Page Range
p. 225-228.
Report number
ESA-SP--281

Conference

Title
Celebratory symposium on a decade of UV astronomy with the IUE satellite.
Dates
12-15 Apr 1988.
Place
Greenbelt, MD (USA).

INIS

Country of Publication
France
Country of Input or Organization
France
INIS RN
20054401
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
ACCRETION DISKS; BINARY STARS; ULTRAVIOLET SPECTRA
Descriptors DEC
SPECTRA; STARS

Optional Information