Outburst spectra of 11 dwarf novae

Details Outburst spectra of 11 dwarf novae Outburst spectra of 11 dwarf novae

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apjs...73..441s&link_type=abstract

Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 73, July 1990, p. 441-459.

Astronomy and Astrophysics

Astrophysics

22

Binary Stars, Cataclysmic Variables, Dwarf Novae, Stellar Mass Accretion, Stellar Spectra, Absorption Spectra, Emission Spectra, Line Spectra, Stellar Orbits

Scientific paper

Medium-resolution spectra of 11 dwarf novae from within 0-5 days after the peak of an outburst are presented. The results are used to study the development and origin of the emission-line core compared with the broad absorption-line wings. Data from eleven systems are summarized and added to previously published data from IR Gem and IP Peg. The data suggest that there is a prominent inner-disk disturbance for outbursting dwarf novae in the 4-5 hr orbital period range.

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