Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995apj...440l..73b&link_type=abstract
Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 440, no. 2, p. L73-L76
Astronomy and Astrophysics
Astronomy
20
Astronomical Photography, Black Holes (Astronomy), Light (Visible Radiation), Novae, X Ray Stars, Accretion Disks, Heat Transfer, Light Curve, Mass Flow, Stellar Spectra
Scientific paper
We present optical observations of a recent X-ray nova considered to be a strong black hole candidate. We observed Nova Velorum 1993 intermittently between 150 and 205 days after the initial outburst and find evidence for a secondary outburst and repeated 'mini-outburst,' similar to those observed from X-ray Nova Persei 1992. A finding chart is presented for this object, as well as spectra of the source at two different epochs. It seems likely that an explanation of the light curve will require consideration of the complex interplay between accretion, mass flow, and X-ray heating effects in the accretion disk and the secondary star.
Bailyn Charles D.
Orosz Jerome A.
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