S147 - A K-type symbiotic star in the LMC

Details S147 - A K-type symbiotic star in the LMC S147 - A K-type symbiotic star in the LMC

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.234.1005m&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 234, Oct. 15, 1988, p. 1005-1010.

Astronomy and Astrophysics

Astronomy

9

K Stars, Magellanic Clouds, Symbiotic Stars, Asymptotic Giant Branch Stars, Carbon Stars, Stellar Luminosity, Stellar Spectra, White Dwarf Stars

Scientific paper

The authors have discovered the first example of an oxygen-rich
symbiotic star in the Large Magellanic Cloud. They show that it involves
an asymptotic branch K5 giant. If the unidentified emission bands at
6830, 7088 Å can be taken as evidence of a white dwarf, then the
hot component is likely to be accreting from the wind of the giant.

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