IAFE   05512
INSTITUTO DE ASTRONOMIA Y FISICA DEL ESPACIO
Unidad Ejecutora - UE
artículos
Título:
CCD BVI photometry and Coravel observations of stars in the open cluster NGC2489
Autor/es:
PIATTI, ANDRÉS E.; CLARIA OLMEDO, JUAN JOSÉ; MERMILLIOD, J.C.; PARISI, M.C.; AHUMADA, A.V.
Revista:
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Referencias:
Año: 2007 vol. 377 p. 1737 - 1746
ISSN:
0035-8711
Resumen:
We present CCD BVI photometry for the southern open cluster NGC2489 and
its surrounding field. The sample consists of 2182 stars measured in an
area of 13.6 × 13.6 arcmin2, extending down to V ~
21.5. These data are supplemented with CORAVEL radial-velocity
observations for seven red giant candidates. A cluster angular radius of
6.7 +/- 0.6 arcmin, equivalent to 3.5 +/- 0.3 pc, is estimated from star
counts carried out inside and outside the cluster region. The comparison
of the cluster colour-magnitude diagrams with isochrones of the Padova
group yields E(B - V) = 0.30 +/- 0.05, E(V - I) = 0.40 +/- 0.05 and V -
MV = 12.20 +/- 0.25 for log t = 8.70 (t =
500+130-100 Myr) and Z = 0.019. NGC2489 is then
located at 1.8 +/- 0.3 kpc from the Sun and 25 pc below the Galactic
plane. The analysis of the kinematical data allowed us to confirm
cluster membership for six red giants, one of them being a spectroscopic
binary. A mean radial velocity of 38.13 +/- 0.33 km s-1 was
derived for the cluster red giants. The properties of a sample of open
clusters aligned along the line of sight of NGC2489 are examined.