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Photometry and period behavior of select W UMA type stars
As stated by Binnendijk (1970, Vistas Astr., 12, 217), the W Ursae Majoris systems are eclipsing variable stars whose light curves have maxima which are strongly curved and minima which are nearly equal in depth. These systems are also spectroscopic double stars and the spectra usually contain absorption lines from both components.
New interpretations on the variations of V651 Mon
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uvby-β photoelectric photometry of the open cluster NGC 6823
Ayuda Buscar en la ayuda Buscar en la ayuda uvby–β photoelectric photometry of the open cluster NGC 6823 J. H. Peña [1] ; A. García-Cole [2] ; M. A. Hobart [3] ; C. de la Cruz [3] ; J. C. Plascencia [4] ; R. Peniche [1] [1] Instituto de Astronomía, Universidad Nacional Autónoma de México (UNAM), México. [2] CCH Sur, UNAM, México. [3] Facultad de Física, Universidad Veracruzana, México. [4] Facultad de Ciencias, UNAM, México. Localización: Revista mexicana de astronomía y astrofísica, ISSN-e 0185-1101, Vol.
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