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- W3201715844 abstract "It is shown that in high-temperature stars in which high speed mass loss is occurring, the rapidly recombining plasma in the stellar envelope can act as an amplifying medium. Model calculations for laser action in Heii λ4686, using the collisional-radiative model, are presented. Menzel's hypothesis of laser action in distended stellar atmospheres is shown to be fully substantiated. The relevance of these results in resolving the problem of intensity anomalies in the spectra of Wolf-Rayet stars is pointed out." @default.
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- W3201715844 date "1975-09-01" @default.
- W3201715844 modified "2023-09-23" @default.
- W3201715844 title "Laser Action in Stellar Envelopes" @default.
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