High galactic latitude RASS X-ray sources. II. (Beuermann+, 1999)

Details High galactic latitude RASS X-ray sources. II. (Beuermann+, 1999) High galactic latitude RASS X-ray sources. II. (Beuermann+, 1999)

Jul 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ycat..33470047b&link_type=abstract

VizieR On-line Data Catalog: J/A+A/347/47. Originally published in: 1999A&A...347...47B

Other

X-Ray Sources, Cross Identifications

Scientific paper

We present a summary of spectroscopic identifications of bright soft high galactic latitude X-ray sources from the ROSAT All-Sky Survey with total PSPC count rates 0.11=0.5cts/s presented previously. Spectroscopic identifications are presented for 70 of 77 sources, 5 sources are identified by other means, and subsidiary information is given for 2 as yet unidentified sources. In practically all cases, a unique optical counterpart exists. As for the brighter fraction of the sample, the largest source classes are Seyfert 1 galaxies, magnetic cataclysmic variables, and hot white dwarfs. In the Galactic Pole caps at |b|>400, Seyfert galaxies dominate, whereas at intermediate latitudes galactic objects as magnetic cataclysmic variables and white dwarfs become relatively more frequent.
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