Ultraviolet orbital variability of the intermediate polars

Details Ultraviolet orbital variability of the intermediate polars Ultraviolet orbital variability of the intermediate polars

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.218..431m&link_type=abstract

In ESA 4th European IUE Conf. p 431-434 (SEE N84-35135 24-88)

Other

2

Periodic Variations, Stellar Spectra, Ultraviolet Spectra, X Ray Sources, Binary Stars, Magnetic Stars, Stellar Mass Accretion, Stellar Motions, White Dwarf Stars, X Ray Binaries

Scientific paper

The variability with orbital phase of the ultraviolet spectrum of the intermediate polars 2A0526-328 (TV Col), 3A0729+103, 4U1849-31 (V1223 Sgr), H2215-086 and H2252-035 (Ao Psc) is analyzed. Intermediate polars are suggested to be close X-ray binaries with a weakly magnetized white dwarf, in which an accretion column and an accretion disk could exist. The presence of an ultraviolet orbital modulation of the continuum and emission lines is discussed in terms of an X-ray heating. Other variable contributions are also present and affect the detection of the orbital modulation.

Affiliated with

Also associated with

No associations

Rating

Ultraviolet orbital variability of the intermediate polars 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 Ultraviolet orbital variability of the intermediate polars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ultraviolet orbital variability of the intermediate polars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1705969