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- W134749063 abstract "One LMC and two SMC fields of 0.3 sq. deg. have been searched for red variables. Carbon stars of V ~ 16–17 are common and are usually of small amplitude, while the LMC alone contains numerous faint M type variables of small amplitude. M giants of small amplitude generally have much shorter periods than carbon stars. The LMC contains numerous Miras with a P-L relation similar to that of galactic Miras, while the SMC has few Miras but many bright red variables of large amplitude which have a steeper P-L relation." @default.
- W134749063 created "2016-06-24" @default.
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- W134749063 date "1984-01-01" @default.
- W134749063 modified "2023-10-17" @default.
- W134749063 title "A Survey for Red Variables in the Magellanic Clouds" @default.
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- W134749063 doi "https://doi.org/10.1017/s0074180900040195" @default.
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