Recovery of the Classical Nova Ar-Circini

Details Recovery of the Classical Nova Ar-Circini Recovery of the Classical Nova Ar-Circini

Nov 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993mnras.265l...9d&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 265, NO. 1/NOV1, P. L9, 1993

Astronomy and Astrophysics

Astronomy

3

Stars: Individual: Ar Cir - Novae, Cataclysmic Variables

Scientific paper

Nova AR Cir (1906) is shown to be an optical pair with a separation of
3.1 arcsec, composed of a 14-mag K3V star and the 18-mag ex-nova. The
light curve and amplitude are compatible with AR Cir being a slow
classical nova.

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