Soft X-ray emission from 2A 0311-227, an AM Herculis-type system

Details Soft X-ray emission from 2A 0311-227, an AM Herculis-type system Soft X-ray emission from 2A 0311-227, an AM Herculis-type system

Aug 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...232l..25c&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 232, Aug. 15, 1979, p. L25, L26. Research supported by the Miller In

Astronomy and Astrophysics

Astronomy

17

Magnetic Stars, Spaceborne Astronomy, Variable Stars, X Ray Sources, X Ray Stars, Binary Stars, Heao 2, Stellar Temperature, X Ray Spectra

Scientific paper

The low-energy detectors on board the HEAO 1 satellite have observed a variable soft X-ray source consistent with the location of 2A 0311-227. The maximum observed intensity is about 2 x 10 to the -11th erg/sq cm-sec. (0.18-0.43 keV) and the temperature must be less than 10 million K. The source is interpreted as a member of the AM Herculis class on the basis of the optical identification with a magnetic binary system.

Affiliated with

Also associated with

No associations

Rating

Soft X-ray emission from 2A 0311-227, an AM Herculis-type system 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 Soft X-ray emission from 2A 0311-227, an AM Herculis-type system, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Soft X-ray emission from 2A 0311-227, an AM Herculis-type system will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1483792