Shock wave interpretation of emission lines in long period variable stars. II - Periodicity and mass loss

An analytical description of strictly periodic shock waves passing through a stellar atmosphere is developed which allows predictions to be made of the onset of instability of the system against mass loss by hydrodynamic ejection. This diagnostic method for determining when shock-driven mass loss ma...

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Veröffentlicht in:	Astrophys. J.; (United States) 1979-03, Vol.228, p.854
Hauptverfasser:	Willson, L. A., Hill, S. J.
Format:	Artikel
Sprache:	eng
Schlagworte:	640102 - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources ATMOSPHERES CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS FLUID MECHANICS GRAVITATION HYDRODYNAMICS INSTABILITY MATHEMATICAL MODELS MECHANICS PULSATIONS SHOCK WAVES STAR MODELS STARS STELLAR ATMOSPHERES VARIABLE STARS
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