Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pasp..100..362s&link_type=abstract
Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 100, March 1988, p. 362-370.
Astronomy and Astrophysics
Astronomy
11
Cataclysmic Variables, Novae, Ultraviolet Astronomy, White Dwarf Stars, Emission Spectra, Iue, Mass Flow Rate, Stellar Mass Accretion, Stellar Temperature
Scientific paper
The authors have obtained IUE low dispersion observations of one nova-like system (V794 Aql) and two AM Her systems (MR Ser and AN UMa) during low or intermediate low accretion rate states. The decreased UV emission during these times was used to place limits on the white dwarf temperatures. When these results are added to the existing data on white dwarf temperatures, it appears that the white dwarfs in systems with normal high accretion rates and only occasional low accretion rate states remain hotter than the white dwarfs in systems with low average accretion rates.
Downes Ronald
Mateo Mario
Szkody Paula
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