A Search for 100micron and Sub-mm Emission in Dwarf Novae

Details A Search for 100micron and Sub-mm Emission in Dwarf Novae A Search for 100micron and Sub-mm Emission in Dwarf Novae

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aj....111..899h&link_type=abstract

Astronomical Journal v.111, p.899

Astronomy and Astrophysics

Astronomy

6

Cataclysmic Variables, Infrared: Stars, Radio Lines: Stars

Scientific paper

Harrison & Gerhz [Al, 103, 243 (1992)] noted that IRAS had apparently detected a few quiescent dwarf novae at 100 μm. This possible detection was intriguing as dwarf novae were not anticipated to be emitters of such long-wavelength radiation. In order to confirm or place limits on this emission, we have undertaken a reanalysis of the IRAS database for four of their "100 μm" dwarf novae. We have also made preliminary sub-mm radio observations of three additional dwarf novae. We find null detections for all our sources in both the IRAS database and in the sub-mm radio range.

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