Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...205.2218w&link_type=abstract
American Astronomical Society Meeting 205, #22.18; Bulletin of the American Astronomical Society, Vol. 36, p.1381
Astronomy and Astrophysics
Astronomy
Scientific paper
M34 is a thoroughly studied open cluster on its way to becoming a fundamental WOCS cluster. We provide photometry of M34 in the U, B, V, R, and I filters in order to re-evaluate its fundamental properties. Observations were made on the WIYN 0.9m telescope on 17 January 2003 using a field of 20' x 20' on the S2KB CCD. PSF photometry was applied using DAOPHOT II and IRAF. We discuss the reddening and metallicity, which were derived using all of the U-B, U-V, U-R, and U-I vs B-V color-color diagrams. We also discuss the distance modulus and age, which were derived from application of Yale-Yonsei isochrones. This work has been supported by the National Science Foundation under Grants AST-0206202 (to CPD), AST-1039617 (REU site at Indiana U.) and by the National Space Grant College and Fellowship Program as a Wisconsin Space Grant Consortium undergraduate scholar (to HG).
Deliyannis Constantine P.
Gneiser H.
Platais Imants
Sarajedini Ata
Windschitl Jessica L.
No associations
LandOfFree
WIYN Open Cluster Study: UBVRI CCD Photometry of M34 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 WIYN Open Cluster Study: UBVRI CCD Photometry of M34, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and WIYN Open Cluster Study: UBVRI CCD Photometry of M34 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1636664