A Possible Detected Faint Shell of the Classical Nova QZ Aurigae

Details A Possible Detected Faint Shell of the Classical Nova QZ Aurigae A Possible Detected Faint Shell of the Classical Nova QZ Aurigae

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aipc..637..548e&link_type=abstract

CLASSICAL NOVA EXPLOSIONS: International Conference on Classical Nova Explosions. AIP Conference Proceedings, Volume 637, pp. 5

Other

Novae, Dwarf Novae, Recurrent Novae, And Other Cataclysmic Variables, Circumstellar Shells, Clouds, And Expanding Envelopes, Circumstellar Masers

Scientific paper

We observed the faint shell of QZ Aur (Nova Aurigae 1964) nearly 30 years of its outburst. Despite a diameter of 0.55+0.12-0.16 arcsec of the intrinsic point source of QZ Aur, a narrow-band Hα image shows that the diameter of the nova shell in 1995 was 0.86+0.14-0.17 arcsec. This rather faint shell exists for a nova suggests that QZ Aur is an object worthy of further study.

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