The UV variability of T CR B

Details The UV variability of T CR B The UV variability of T CR B

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982esasp.176..229c&link_type=abstract

In its 3rd European IUE Conf. p 229-231 (SEE N83-11889 02-88)

Computer Science

15

Corona Borealis Constellation, Novae, Ultraviolet Spectra, Variability, Companion Stars, Continuums, High Temperature Plasmas, Line Spectra, Stellar Luminosity

Scientific paper

The continuum and rich emission line spectrum during the activity phase of T Cr B are discussed. Features of the UV continuum include a flat spectrum in Mar 1979, regular increase of the integrated luminosity and UV excess from Mar 1979 to Feb 1981, and decay of the integrated flux from Feb to Dec 1981. The overall appearance of the emission line spectrum indicates the presence of a high temperature plasma in which most of the lines (except He II) are collisionally excited. The lines are generally stronger when the continuum is stronger.

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