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- W196369312 abstract "Detailed spectroscopic work has begun for several stars that have been classified WN 7. All show absorption lines in the upper Balmer series and in ionized helium. The absolute magnitudes, established from cluster membership, are relatively brighter than those of most other WR stars. In this paper the outflow velocity near the stellar photosphere is shown to be similar to that in Of stars. These WN 7 stars show somewhat larger emission line widths and probably have less hydrogen in their envelopes, but otherwise have similar luminosities and temperatures as Of stars." @default.
- W196369312 created "2016-06-24" @default.
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- W196369312 date "1978-01-01" @default.
- W196369312 modified "2023-09-28" @default.
- W196369312 title "Evolution of Massive Stars: When Does an of Star Become a WR Star?" @default.
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- W196369312 doi "https://doi.org/10.1017/s0074180900145784" @default.
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