From the analysis of the galactic counterparts of the HS variables, η Car, AG Car and P Cyg we conclude that their atmospheres are near critical physical conditions so that small changes of the mass outflow could produce a large variation of the atmospheric structure and nova-like explosions at nearly constant Mbo1.

Viotti, R., Rossi, L., Altamore, A., Rossi, C., Baratta G., B., Cassatella, A. (1988). Atmospheric phenomena in ETA carinae and the Hubble-Sandage variables. In Atmospheric Diagnostics of Stellar Evolution. Chemical Peculiarity, Mass Loss, and Explosion. (pp.127) [10.1007/BFb0034569].

Atmospheric phenomena in ETA carinae and the Hubble-Sandage variables

ALTAMORE, Aldo;
1988-01-01

Abstract

From the analysis of the galactic counterparts of the HS variables, η Car, AG Car and P Cyg we conclude that their atmospheres are near critical physical conditions so that small changes of the mass outflow could produce a large variation of the atmospheric structure and nova-like explosions at nearly constant Mbo1.
Viotti, R., Rossi, L., Altamore, A., Rossi, C., Baratta G., B., Cassatella, A. (1988). Atmospheric phenomena in ETA carinae and the Hubble-Sandage variables. In Atmospheric Diagnostics of Stellar Evolution. Chemical Peculiarity, Mass Loss, and Explosion. (pp.127) [10.1007/BFb0034569].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11590/171730
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