Light variations and angular momentum loss from the He-strong magnetic chemically peculiar star HD 37776

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dc.creatorMikulasek, Zdenek
dc.creatorKrticka, Jiri
dc.creatorZverko, Juraj
dc.creatorZiznovsky, Jozef
dc.creatorJanik, Jan
dc.date2005-09-26
dc.date.accessioned2026-07-07T06:18:57Z
dc.date.available2026-07-07T06:18:57Z
dc.descriptionWe present a principle component analysis of multicolour light variations of the He-strong magnetic chemically peculiar star HD 37776 and its (O-C) diagram. The period increase rate found, (dP/dt) / P = 5.5 x 10^{-6}/year, is consistent with the conception of angular momentum loss through magnetically confined stellar wind.
dc.description3 pages; to appear in the proceedings of Active OB-Stars: Laboratories for Stellar & Circumstellar Physics, S. Stefl, S. Owocki and A. Okazaki eds
dc.identifierhttps://arxiv.org/abs/astro-ph/0509751
dc.identifierhttp://arxiv.org/abs/astro-ph/0509751
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/94914
dc.subjectAstrophysics
dc.titleLight variations and angular momentum loss from the He-strong magnetic chemically peculiar star HD 37776
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