The optical identification of H2252-035 with a cataclysmic variable

Details The optical identification of H2252-035 with a cataclysmic variable The optical identification of H2252-035 with a cataclysmic variable

Nov 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.193p..25g&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 193, Nov. 1980, p. 25P-33P. Research supported by the Science Research

Astronomy and Astrophysics

Astronomy

7

Binary Stars, Stellar Mass Accretion, Stellar Spectrophotometry, Variable Stars, White Dwarf Stars, X Ray Sources, Emission Spectra, Heao 3, Novae, Position (Location), Sky Surveys (Astronomy), Stellar Magnitude

Scientific paper

An improved position is presented for the X-ray source H2252-033 using the Ariel V Sky Survey Instrument, and precise positioning using the Scanning Modulation Collimator on HEAO-1. The source is identified optically with a 13th magnitude emission-line object, which is probably a white dwarf binary with a well formed accretion disk, with similarities to the dwarf novae (e.g., SS Cyg) at minimum.

Affiliated with

Also associated with

No associations

Rating

The optical identification of H2252-035 with a cataclysmic variable 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 The optical identification of H2252-035 with a cataclysmic variable, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The optical identification of H2252-035 with a cataclysmic variable will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1391888