Steam in RX Puppis

Details Steam in RX Puppis Steam in RX Puppis

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mnras.187..813b&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 187, June 1979, p. 813-816.

Astronomy and Astrophysics

Astronomy

16

Absorption Spectra, Astronomical Spectroscopy, Binary Stars, Stellar Models, Variable Stars, Water, B Stars, Giant Stars, Line Spectra, Mira Variables, Thermal Radiation

Scientific paper

The presence of H2O and CO absorption in RX Puppis is demonstrated by means of 2-micron spectroscopy. The existence of a Mira variable in this star is thereby confirmed. These data are not easily reconciled with a recent model in which a single B giant is invoked as the central energy source. Instead, it is suggested that RX Pup is explicable in terms of a symbiotic binary model.

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