The X-ray spectrum of emission line stars (superluminous and symbiotic)

Details The X-ray spectrum of emission line stars (superluminous and symbiotic) The X-ray spectrum of emission line stars (superluminous and symbiotic)

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985esasp.239...95b&link_type=abstract

In ESA Proceedings of ESA Workshop on a Cosmic X-Ray Spectroscopy Mission p 95-98 (SEE N86-22461 12-89)

Physics

3

Line Spectra, Stellar Spectra, Symbiotic Stars, X Ray Spectra, Exosat Satellite, High Temperature Plasmas, Stellar Temperature, Stellar Winds

Scientific paper

The observation of the X-ray spectrum of peculiar emission line stars, whose atmospheric envelopes are characterized by extreme physical conditions, represents an important tool to investigate the processes of formation of high temperature plasmas. The authors discuss the case of the superluminous object η Car showing both high and low temperature regions and an asymmetric wind. They present new EXOSAT observations of symbiotic stars. AG Draconis observed at a minimum phase shows a low temperature X-ray spectrum. A weak flux from the Mira variable R Aqr observed near maximum has been also detected.

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