The SMC Cluster NGC330
نویسندگان
چکیده
منابع مشابه
SPB stars in the open SMC cluster NGC 371
Pulsation in β Cep and SPB stars are driven by the κ mechanism which depends critically on the metallicity. It has therefore been suggested that β Cep and SPB stars should be rare in the Magellanic Clouds which have lower metallicities than the solar neighborhood. To test this prediction we have observed the open SMC cluster NGC 371 for 12 nights in order to search for β Cep and SPB stars. Surp...
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ژورنال
عنوان ژورنال: Symposium - International Astronomical Union
سال: 1980
ISSN: 0074-1809
DOI: 10.1017/s0074180900092147