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| Membership of low-mass stars in the open cluster Alpha Persei The results of a combined astrometric, photometric, and spectroscopicsearch for low-mass members in the intermediate-age open cluster AlphaPersei are presented. Over 130 low-mass new members have been identifiedto M(v) about 12.5, almost doubling the previous number of knownmembers. The new membership information suggests a slight upwardrevision of Alpha Per's age to about 8 x 10 exp 7 yr. Alpha Per isnoticeably spatially elongated in a direction parallel to the Galacticplane, most likely due to tidal deformation. Analysis of thedistribution of relative H-alpha emission strengths among Alpha Permembers confirms the view that the mean H-alpha strength decreases inincreasingly older systems. Allowing for survey incompleteness, onecannot reject the idea that the luminosity function is consistent withthe field luminosity function to M(v) about 9 or 10.
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Membre dels grups següents:
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Dades d'Observació i Astrometria
Constel·lació: | Perseus |
Ascensió Recta: | 03h40m56.48s |
Declinació: | +49°30'22.2" |
Magnitud Aparent: | 9.9 |
Moviment propi RA: | 3.9 |
Moviment propi Dec: | -4.6 |
B-T magnitude: | 10.011 |
V-T magnitude: | 9.91 |
Catàlegs i designacions:
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