Cataclysmic Binaries: Classical and Recurrent Novae

Details Cataclysmic Binaries: Classical and Recurrent Novae Cataclysmic Binaries: Classical and Recurrent Novae

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000eaa..booke1622w&link_type=abstract

"Encyclopedia of Astronomy and Astrophysics, Edited by Paul Murdin, article 1622. Bristol: Institute of Physics Publishing, 2001

Astronomy and Astrophysics

Astrophysics

Stars, Binary Stars

Scientific paper

The Latin word nova, meaning `new', was applied historically to the sudden appearance of a bright star, not previously recorded. Such novae stellae appear in Eastern records from about 1500 BC and in European records in the past three centuries (many, however, are ancient SUPERNOVAE). The discovery of a different kind of nova, dwarf novae, in the mid-nineteenth century, led to the use of classica...

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