Observation of continuum emission between 1 and 4 MM from the carbon star V Cygni

Details Observation of continuum emission between 1 and 4 MM from the carbon star V Cygni Observation of continuum emission between 1 and 4 MM from the carbon star V Cygni

Aug 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....77..155q&link_type=abstract

Astronomy and Astrophysics, vol. 77, no. 1-2, Aug. 1979, p. 155-158.

Astronomy and Astrophysics

Astronomy

4

Carbon Stars, Continuous Radiation, Millimeter Waves, Near Infrared Radiation, Radio Sources (Astronomy), Stellar Envelopes, Far Infrared Radiation, Line Spectra, Mass Transfer, Molecular Spectra, Radiant Flux Density, Radio Emission, Stellar Mass

Scientific paper

A flux density of 15 plus or minus 5 Jy has been detected at a mean wavelength of 1.5 mm from the dusty circumstellar envelope of the Mira N-type star, V Cygni. An interpretation of this high continuum emission is attempted on the basis of the near-infrared flux and of predicted flux in the far-infrared and millimeter regions, together with a comparison with the star IRC plus 10216. Shock waves and consequent mass-loss phenomena known to take place in the atmosphere of the Mira variable stars should support the assumption of a flarelike event.

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