Imaging of the Possible Nebula around the Cataclysmic Variable V1101 Aquilae

Details Imaging of the Possible Nebula around the Cataclysmic Variable V1101 Aquilae Imaging of the Possible Nebula around the Cataclysmic Variable V1101 Aquilae

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000pasp..112.1212d&link_type=abstract

The Publications of the Astronomical Society of the Pacific, Volume 112, Issue 775, pp. 1212-1214.

Astronomy and Astrophysics

Astronomy

Stars: Novae, Cataclysmic Variables, Stars: Individual (V1101 Aquilae)

Scientific paper

I have obtained Hα and [O III] λ5007 imaging observations of the cataclysmic variable V1101 Aql to study the nearby nebulosity recently reported by N. Masetti and M. Della Valle. My images reveal only the southern half of the nebulosity and find that it is not an emission-line source, but it is likely a mid-G star. The northern part of the suspected nebulosity, if real, is likely a variable source unrelated to the southern object.

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