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.
Baratta G., B., Piro, L., Viotti, R., Cassatella, A., Altamore, A., Ricciardi, O., et al. (1985). The X-ray spectrum of emission line stars (superluminous and symbiotic). In Proceedings of ESA Workshop on a Cosmic X-Ray Spectroscopy Mission (pp.95-98). NOORDWIJK : European Space Agency Publications.
The X-ray spectrum of emission line stars (superluminous and symbiotic)
ALTAMORE, Aldo;
1985-01-01
Abstract
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.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
