Spectroscopy of poorly known northern dwarf novae. II

Details Spectroscopy of poorly known northern dwarf novae. II Spectroscopy of poorly known northern dwarf novae. II

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26as...93..419b&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 93, no. 3, June 1992, p. 419-439. Research supported by DFG.

Astronomy and Astrophysics

Astrophysics

22

Astronomical Catalogs, Dwarf Novae, Northern Sky, Stellar Spectra, Stellar Spectrophotometry, Variable Stars, Binary Stars, Cataclysmic Variables, Emission Spectra

Scientific paper

A spectrophotometric study of faint northern dwarf nova candidates is presented. A detailed account of previous knowledge of the individual systems is given along with a critical examination of the newly obtained spectra. Measurements of equivalent widths, line strengths, and line widths of the emission lines are discussed. While the results verify the dwarf nova classification in most cases, there are some notable exceptions. Among these is a group of three M stars (HN Cyg, UY Vul, and UZ Vul). MR Per is found to be a main sequence M star.

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