First Spectroscopy of the Dwarf Nova KX Aql: a Possible New SU UMa System

Details First Spectroscopy of the Dwarf Nova KX Aql: a Possible New SU UMa System First Spectroscopy of the Dwarf Nova KX Aql: a Possible New SU UMa System

Jun 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ibvs.5101....1t&link_type=abstract

Information Bulletin on Variable Stars, 5101, 1.

Physics

4

Spectroscopy

Scientific paper

We present the quiescence spectrum of the dwarf nova KX Aql. The most
prominent spectral features are the extremely strong Balmer emission
lines, indicative of a dwarf nova at a low mass-transfer rate. The
absence of secondary absorption and a large outburst amplitude suggests
KX Aql as a member of the SU UMa subclass.

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