A dust excess in Nova Cygni 1975?

Details A dust excess in Nova Cygni 1975? A dust excess in Nova Cygni 1975?

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...151..452b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 151, no. 2, Oct. 1985, p. 452-454.

Astronomy and Astrophysics

Astrophysics

4

Cosmic Dust, Infrared Photometry, Interstellar Matter, Cygnus Constellation, Infrared Radiation, Novae

Scientific paper

The "dustless" Nova Cygni 1975 (V1500 Cyg) had an excess at 10 μm after ≡100 days. The authors show that the behaviour of this excess is consistent with the heating of dust close to the nova during eruption. Similar effects in future novae might usefully be investigated by means of co-ordinated searches for optical "light-echo" effects and suitable mapping at infrared wavelengths.

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