INVESTIGADORES
AHUMADA Andrea Veronica
artículos
Título:
A CCD BVI Photometric Study of the Young, Highly Reddened Open Cluster NGC 6318
Autor/es:
PIATTI, ANDRÉS E.; CLARIÁ, JUAN J.; AHUMADA, ANDREA V.
Revista:
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC
Editorial:
UNIV CHICAGO PRESS
Referencias:
Lugar: Chicago; Año: 2005 vol. 117 p. 22 - 31
ISSN:
0004-6280
Resumen:
We present CCD BVI photometry for the southern open cluster NGC 6318.
The sample consists of 9876 stars measured in an area of
13.6m×13.6m, extending down to V~21.5 mag. Star counts carried out
within and outside the cluster region allowed us to estimate the cluster
angular radius as ~8'. The comparison of the cluster color-magnitude
diagrams with isochrones of the Geneva group yields E(B-V)=1.20+/-0.05,
E(V-I)=1.55+/-0.10, and V-MV=15.45+/-0.35 for logt=8.20
(t=160 Myr) and Z=0.020. NGC 6318 is then located at 2.1+/-0.5 kpc from
the Sun and 30 pc below the Galactic plane. Using the WEBDA open cluster
database, we examined the structure of the Galactic disk along the line
of sight of NGC 6318. Among the known clusters in this direction, HM 1
and BH 222 are the farthest ones, while those located between 1 and 2
kpc of the Sun appear to be more absorbed than those expected to follow
a quasi-linear extinction law.