PQT 080119:091534+081356 is a probable dwarf nova near maximum

Details PQT 080119:091534+081356 is a probable dwarf nova near maximum PQT 080119:091534+081356 is a probable dwarf nova near maximum

Jan 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1367....1g&link_type=abstract

The Astronomer's Telegram, #1367

Astronomy and Astrophysics

Astronomy

1

Optical, Cataclysmic Variables, Novae, Transients

Scientific paper

Spectra of the transient PQT080119:091534+081356 (Donalek et al., ATEL #1362) obtained at the Palomar 200-inch Hale telescope on 20 Jan 2008 UT show strong Balmer lines (beta through zeta, and possibly higher) in absorption, superposed on a fairly blue continuum; the H alpha line may be just filled by associated emission; and there is a possible weak absorption line of He I 4471. All are at a zero redshift, within the measuring uncertainties.

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