HD 52452: New BVRI Photometry

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dc.creatorBarway, Sudhanshu
dc.creatorPandey, S. K.
dc.date2004-08-19
dc.date.accessioned2026-07-07T02:14:20Z
dc.date.available2026-07-07T02:14:20Z
dc.descriptionIn this paper we report the multi-band BVRI photometry of HD 52452. The comparison of our data with previous observations reported by Messina et al. (2001) shows that there is a variation in amplitude, but the phases of the two minima, thus the positions of the spot, are quite stable during our observations.
dc.description4 pages, 2 figures, IBVS No. 5553, 1
dc.identifierhttps://arxiv.org/abs/astro-ph/0408351
dc.identifierhttp://arxiv.org/abs/astro-ph/0408351
dc.identifierInform.Bull.Var.Stars 5553 (2004) 1
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8073
dc.subjectAstrophysics
dc.titleHD 52452: New BVRI Photometry
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