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PERIODIC RADIO CONTINUUM EMISSION ASSOCIATED WITH THE β CEPHEI STAR V2187 CYG
We present new optical time-resolved photometry and medium-resolution spectroscopy of V2187 Cyg. We confirm its classification as a β Cephei star based on sinusoidal light variations with a period of 0.2539 days and mean amplitudes of 0.037 and 0.042 magnitudes in i and V , respectively. We classifi...
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Publicado no: | Revista Mexicana de Astronomía y Astrofísica |
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Main Authors: | , , , , , , |
Formato: | Artigo |
Idioma: | Inglês |
Publicado em: |
Universidad Nacional Autónoma de México
2014
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Assuntos: | |
Acesso em linha: | https://www.redalyc.org/articulo.oa?id=57131044015 |
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