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- W3078182247 abstract "Abstract A physical mechanism that can result in the generation of extended expanding atmospheres is discussed. The process involves the unloading of stellar material following the arrival of a shock wave at the edge of the star. The basic principles are developed from a discussion of a simplified case that has been studied in the laboratory; they are then applied to the atmosphere of a star. A radiation-hydrodynamics computation of a model cepheid is then used to obtain quantitative atmospheric profiles. The computed continuum and spectral lines during the unloading process are then examined. A discussion of the possibility that the unloading process occurs in stars other than cepheids suggests the existence of a shock visibility factor associated with ionization or dissociation in the region behind the shock front and leads to a possible alternate interpretation of the variable star instability strips in the H-R diagram." @default.
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- W3078182247 date "1970-08-01" @default.
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- W3078182247 title "A Physical Mechanism for the Generation of Extended Stellar Atmospheres" @default.
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- W3078182247 doi "https://doi.org/10.1017/s0252921100151334" @default.
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