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MULTICOLOR U BV RI POLARIMETRY OF NGC 4755 AND THE B CEPHEI POPULATION

We present U BV RI polarimetric observations of 66 stars in the direction of NGG 4755, including eleven β cephei stars. About half of these variables show indications of intrinsic polarization, but according to the theory neither radial nor non-radial pulsations could cause such polarizations. From...

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Publikašuvnnas:Revista Mexicana de Astronomía y Astrofísica
Váldodahkkit: E. Irene Vega, Ana María Orsatti, Ruben E. Martínez
Materiálatiipa: Artigo
Giella:Inglês
Almmustuhtton: Universidad Nacional Autónoma de México 2015
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Liŋkkat:https://www.redalyc.org/articulo.oa?id=57142745009
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