V 394 CrA - Outburst light curves and notes on its position among the recurrent novae

Details V 394 CrA - Outburst light curves and notes on its position among the recurrent novae V 394 CrA - Outburst light curves and notes on its position among the recurrent novae

May 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...197..148d&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 197, no. 1-2, May 1988, p. 148-150.

Astronomy and Astrophysics

Astrophysics

11

Balmer Series, Cataclysmic Variables, Dwarf Novae, Emission Spectra, Light Curve, Line Spectra, Bursts, H I Regions, H Ii Regions

Scientific paper

The light curves of the recurrent nova V394 CrA during its outbursts of 1949 and 1987 are compared. Identified as a 19m object at minimum, the position of V394 CrA in the amplitude-t3-time diagram indicates a close similarity to U Sco. LS And, V794 Oph, V909 Sgr and MU Ser are candidates to be watched for recurrent nova behaviour. The z-distance of recurrent novae indicates intermediate disk population; the population is certainly different from that of classical novae.

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