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HD 24147


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CP2 stars as viewed by the UVBY H_beta system
The aim of this work is to study the capacity of the uvby H_βsystem for detecting the chemically peculiar (CP) stars based on theeffect that peculiar features in the flux distribution have on all theStromgren-Crawford indices. Our study focuses on the classical magneticpeculiar stars (CP2), though Am stars (CP1) are also included forcomparison with cool CP2 stars. Satisfactory results were obtained forhot CP2 stars: the definition of a new index p, which is a linearcombination of uvby H_β colours, allowed us to separate a highpercentage of hot CP2 stars from normal stars. According to this newindex, 60 new CP2 candidates are proposed. The working sample wasextracted from The General Catalogue of Ap and Am stars by \cite[Rensonet al. (1991)]{ren91}. Photometric observations to enlarge the sample ofCP2 stars with complete uvby H_β photometry were carried out. Theseobservations are also reported in the present paper. The new index p isalso used to correct the reddening of early CP2 stars computed as ifthey were normal stars. Tables 2, 3 and 7 are also available inelectronic form from CDS via anonymous ftp to cdsarc.u-strasbg.fr(130.79.128.5) or via http://cdsweb.u-strasbg.fr/Abstract.html

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Dades d'Observació i Astrometria

Constel·lació:Eridanus
Ascensió Recta:03h50m12.39s
Declinació:-16°38'11.9"
Magnitud Aparent:8.404
Distancia:195.695 parsecs
Moviment propi RA:7.3
Moviment propi Dec:4.8
B-T magnitude:8.691
V-T magnitude:8.428

Catàlegs i designacions:
Noms Propis   (Edit)
HD 1989HD 24147
TYCHO-2 2000TYC 5881-897-1
USNO-A2.0USNO-A2 0675-01318298
HIPHIP 17942

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