2003/10/02 by Brian Warner, Brian D. Warner, P. A. Woudt +3
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysical Phenomena and Observations #Astrophysics (astro-ph) #FOS: Physical sciences #Gamma-ray bursts and supernovae #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0310072
4 pages, 2 figures; to appear in `Variable Stars in the Local Group', eds. Don Kurtz and Karen Pollard
arxiv created 2003/10/02 · openalex publication_date 2003/10/02 · arxiv updated 2009/12/01 · openalex created_date 2022/10/07 · openalex updated_date 2026/07/28
There are now four dwarf novae known with white dwarf primaries that show\nlarge amplitude non-radial oscillations of the kind seen in ZZ Cet stars. We\ncompare the properties of these stars and point out that by the end of the\nSloan Digital Sky Survey more than 30 should be known.\n