PHL 227 - The discovery of a new nova-like object

Details PHL 227 - The discovery of a new nova-like object PHL 227 - The discovery of a new nova-like object

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...149l...4h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 149, no. 1, Aug. 1985, p. L4-L6.

Astronomy and Astrophysics

Astrophysics

14

Cataclysmic Variables, Novae, Stellar Spectra, Ultraviolet Spectra, Absorption Spectra, Line Spectra, Spectral Energy Distribution

Scientific paper

The southern (13.5-mag) subdwarf candidate PHL 227 is found to be a nova-like object (UX UMa star). The line spectrum, both at visual and UV wavelengths, is strikingly similar to that of the well known UX UMa star V3885 Sgr. PHL 227 lies in the sky region of the Palomar Green survey. In this survey only two UX UMa stars (brighter than B = 16.2) sofar have been discovered. Although PHL 227 is brighter than these it seems to have escaped detection.

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