Novae and the R Coronae Borealis phenomenon

Details Novae and the R Coronae Borealis phenomenon Novae and the R Coronae Borealis phenomenon

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988kfnt....4...33r&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 4, Sept.-Oct. 1988, p. 33-38. In Russian.

Astronomy and Astrophysics

Astronomy

6

Cosmic Dust, Novae, R Coronae Borealis Stars, Stellar Spectra, Astronomical Photometry, Infrared Photometry, Light Curve, Stellar Envelopes

Scientific paper

The frequent formation of a dust ring in the main shell whose plane of symmetry coincides with the plane of the orbit of the binary-Nova progenitor is revealed on the basis of visual and IR photometry of 11 Novae. The average radius of the main shell during dust condensation is about 4 x 10 to the 14th cm. If the line of sight passes through the dust ring that has formed, a temporary weakening of the visual light is observed similar to that in R Coronae Borealis-type minima.

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