The Infrared Emission of the Shell around Nova V705 Cassiopeiae 1993

Details The Infrared Emission of the Shell around Nova V705 Cassiopeiae 1993 The Infrared Emission of the Shell around Nova V705 Cassiopeiae 1993

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001pasp..113.1554d&link_type=abstract

The Publications of the Astronomical Society of the Pacific, Volume 113, Issue 790, pp. 1554-1558.

Astronomy and Astrophysics

Astronomy

1

Infrared: Stars, Stars: Novae, Cataclysmic Variables, Stars: Winds, Outflows, Techniques: High Angular Resolution

Scientific paper

The infrared detection of the nova Cas 1993 shell 2513 days after outburst is presented. Broadband (J, H, and K) absolute fluxes for the ejecta are derived after isolating its emission from the central star contribution. A revised expansion distance for this system of d=2.9+/-0.4 kpc is obtained on the basis of the angular size of the envelope. The possible sources for the nebular IR emission are discussed, and a comparison with the previous evolution of the shell is made.

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