Identification of 4U 1849-31 with V1223 Sagittarii and discovery of optical pulsations

Details Identification of 4U 1849-31 with V1223 Sagittarii and discovery of optical pulsations Identification of 4U 1849-31 with V1223 Sagittarii and discovery of optical pulsations

Oct 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...249l..21s&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 249, Oct. 1, 1981, p. L21-L24. Research supported by the Fundacao de

Astronomy and Astrophysics

Astronomy

44

Variable Stars, X Ray Sources, Dwarf Stars, Optical Emission Spectroscopy, Sky Surveys (Astronomy), Spaceborne Astronomy, Stellar Rotation, Stellar Spectrophotometry, X Ray Astronomy, X Ray Spectra

Scientific paper

The X-ray source 4U 1849-31 is identified with the 13 mag star V1223 Sgr, on the basis of a precise HEAO 1 modulation collimator X-ray position uniquely selected by the Ariel-5 sky survey location. It is shown by optical spectroscopy and photometry that V1223 Sgr is a cataclysmic variable, displaying a photometric period of 13.2 min that is interpreted as being due to the rotation of a degenerate dwarf. The similarity of this system to H2252-035 is noted.

Affiliated with

Also associated with

No associations

Rating

Identification of 4U 1849-31 with V1223 Sagittarii and discovery of optical pulsations 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 Identification of 4U 1849-31 with V1223 Sagittarii and discovery of optical pulsations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Identification of 4U 1849-31 with V1223 Sagittarii and discovery of optical pulsations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1468681