Search for dust shells in W Ser binaries and similar objects: KX Andromedae and V367 Cygni

Details Search for dust shells in W Ser binaries and similar objects: KX Andromedae and V367 Cygni Search for dust shells in W Ser binaries and similar objects: KX Andromedae and V367 Cygni

Nov 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997astl...23..704t&link_type=abstract

Astronomy Letters, Volume 23, Issue 6, November 1997, pp.704-708; Pis'ma v Astronomicheskii Zhurnal, Vol. 23, p. 810

Astronomy and Astrophysics

Astronomy

3

Scientific paper

The photometric observations of two strongly interacting W Ser binaries (KX And and V367 Cyg) are analyzed. The spectral classification of the stellar components of the binaries is made, and the nature of excess emission at lambda 3.5 and 5 microns is studied. It is shown that the observed LM excess can be attributed to the emission from disk-shaped ionized shells.

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