Near IR study of the young cluster NGC 2453

Details Near IR study of the young cluster NGC 2453 Near IR study of the young cluster NGC 2453

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001basi...29..329h&link_type=abstract

Bulletin of the Astronomical Society of India, Vol. 29, p. 329-333

Astronomy and Astrophysics

Astronomy

1

Nicmos Camera, Open Clusters, Near-Infrared, Cluster Distance

Scientific paper

In an attempt to understand early phases of stellar evolution and star formation, we have taken up the study of extremely young star clusters in the near infrared wavebands. These clusters are deeply embedded inside the molecular gas and dust but radiate substantially in the infrared. We have observed one such cluster NGC 2453 from Mt Abu Infrared Observatory (MIRO) operated by the Physical Research Laboratory, using the NICMOS-3 infrared array mounted on the 1.2 m Cassegrain focus telescope. The observations were made in the J, H and K? wavebands in February 2000. The data reduction and the photometry has been performed using IRAF. Preliminary results are presented.

Affiliated with

Also associated with

No associations

Rating

Near IR study of the young cluster NGC 2453 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Near IR study of the young cluster NGC 2453, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Near IR study of the young cluster NGC 2453 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1485382