White dwarfs in Be star binary systems

Details White dwarfs in Be star binary systems White dwarfs in Be star binary systems

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...248..139a&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 248, no. 1, Aug. 1991, p. 139, 140.

Astronomy and Astrophysics

Astrophysics

12

B Stars, Binary Stars, Neutron Stars, White Dwarf Stars, X Ray Sources, Stellar Envelopes, Stellar Mass Accretion, X Ray Spectra

Scientific paper

An evaluation is made of possible reasons for the persistent inability to identify white dwarf stars in the Be binary systems. It is noted that many Be stars exhibiting large optical enhancements may be Be + WD and Be + He systems, and that observations of pulsations in the H-alpha emission, as well as observation of time delays between enhancements of optical line and continuum, can identify such systems.

Affiliated with

Also associated with

No associations

Rating

White dwarfs in Be star binary systems does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with White dwarfs in Be star binary systems, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and White dwarfs in Be star binary systems will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1724324