The 1978 outburst of the recurrent nova WZ Sagittae

Details The 1978 outburst of the recurrent nova WZ Sagittae The 1978 outburst of the recurrent nova WZ Sagittae

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987acaps...7..189h&link_type=abstract

(Acta Astrophysica Sinica, vol. 7, 1987, p. 189-194) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 11, Dec. 1987, p.

Physics

Astronomical Photography, Cataclysmic Variables, Novae, Sagittarius Constellation, Stellar Physics, Dwarf Novae, Eclipsing Binary Stars, Periodic Variations, Stellar Magnitude

Scientific paper

The results of photographic observations of the recurrent nova WZ Sge during its 1978 outburst, between December 5 and 25, using the 40/200 cm double astrograph of Beijing Observatory are given. The observed properties are discussed and the total energy released during the outburst is calculated to be about 1.07 (+ 40) erg. It is estimated that the next outburst will occur around the year 2011.

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