Are classical Be stars sources of hard X-rays

Details Are classical Be stars sources of hard X-rays Are classical Be stars sources of hard X-rays

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982iaus...98..353p&link_type=abstract

In: Be stars; Proceedings of the Symposium, Munich, West Germany, April 6-10, 1981. (A83-10301 01-90) Dordrecht, D. Reidel Publi

Astronomy and Astrophysics

Astronomy

15

B Stars, Galactic Radiation, Stellar Luminosity, Stellar Spectrophotometry, X Ray Sources, Binary Stars, Data Bases, Stellar Spectra, X Ray Astronomy

Scientific paper

A point summation technique was used to search the UHURU data base for X-ray emission from classical Be stars. Of the thirty-two stars considered, only three (Gamma Cas, HR 4009, and HD 187399) were detected at the 3.3sigma level or higher. For reasons discussed in this paper, HD 45314, Pi Aqr, Kappa Dra, and 48 Per are considered to be possible detections. The X-ray emission from Gamma Cas from late 1970 through early 1973 is discussed.

Affiliated with

Also associated with

No associations

Rating

Are classical Be stars sources of hard X-rays 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 Are classical Be stars sources of hard X-rays, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Are classical Be stars sources of hard X-rays will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-842041