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An HST/WFPC2 survey of bright young clusters in M 31. IV. Age and mass estimates

Perina, S. and Cohen, J. G. and Barmby, P. and Beasley, M. A. and Bellazzini, M. and Brodie, J. P. and Federici, L. and Fusi Pecci, F. and Galleti, S. and Hodge, P. W. and Huchra, J. P. and Kissler-Patig, M. and Puzia, T. H. and Strader, J. (2010) An HST/WFPC2 survey of bright young clusters in M 31. IV. Age and mass estimates. Astronomy and Astrophysics, 511 . A23. ISSN 0004-6361. https://resolver.caltech.edu/CaltechAUTHORS:20100413-105838778

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Abstract

Aims. We present the main results of an imaging survey of possible young massive clusters (YMC) in M 31 performed with the Wide Field and Planetary Camera 2 (WFPC2) on the Hubble Space Telescope (HST), with the aim of estimating their age and their mass. We obtained shallow (to B ~ 25) photometry of individual stars in 19 clusters (of the 20 targets of the survey). We present the images and color magnitude diagrams (CMDs) of all of our targets. Methods. Point spread function fitting photometry of individual stars was obtained for all the WFPC2 images of the target clusters, and the completeness of the final samples was estimated using extensive sets of artificial stars experiments. The reddening, age, and metallicity of the clusters were estimated by comparing the observed CMDs and luminosity functions (LFs) with theoretical models. Stellar masses were estimated by comparison with theoretical models in the (Age) vs. absolute integrated magnitude plane, using ages estimated from our CMDs and integrated J, H, K magnitudes from 2MASS-6X. Results. Nineteen of the twenty surveyed candidates were confirmed to be real star clusters, while one turned out to be a bright star. Three of the clusters were found not to be good YMC candidates from newly available integrated spectroscopy and were in fact found to be old from their CMD. Of the remaining sixteen clusters, fourteen have ages between 25 Myr and 280 Myr, two have older ages than 500 Myr (lower limits). By including ten other YMC with HST photometry from the literature, we assembled a sample of 25 clusters younger than 1 Gyr, with mass ranging from 0.6 × 10^4 M_☉ to 6 × 10^4 M_☉, with an average of ~3 × 10^4 M_☉. Our estimates of ages and masses well agree with recent independent studies based on integrated spectra. Conclusions. The clusters considered here are confirmed to have masses significantly higher than Galactic open clusters (OC) in the same age range. Our analysis indicates that YMCs are relatively common in all the largest star-forming galaxies of the Local Group, while the lack of known YMC older than 20 Myr in the Milky Way may stem from selection effects.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1051/0004-6361/200913459DOIArticle
https://arxiv.org/abs/0911.3166arXivDiscussion Paper
ORCID:
AuthorORCID
Cohen, J. G.0000-0002-8039-4673
Barmby, P.0000-0003-2767-0090
Bellazzini, M.0000-0001-8200-810X
Brodie, J. P.0000-0002-9658-8763
Puzia, T. H.0000-0003-0350-7061
Strader, J.0000-0002-1468-9668
Additional Information:© 2010 ESO. Received: 13 October 2009; accepted: 5 November 2009. We are grateful to an anonymous referee for a constructive report and for useful suggestions that improved the quality of this paper. S.P. and M.B. acknowledge the financial support of INAF through the PRIN 2007 grant CRA 1.06.10.04 “The local route to galaxy formation...”. P.B. acknowledges research support through a Discovery Grant from the Natural Sciences and Engineering Research Council of Canada. J.G.C. is grateful for partial support through grant HST-GO-10818.01-A from the STcI. T.H.P. gratefully acknowledges support in form of a Plaskett Fellowship at the Herzberg institute of Astrophysics in Victoria, BC. J.S. was supported by NASA through an Hubble Fellowship, administered by STScI. We are grateful to S. van den Bergh for having pointed out some errors in the historical reconstruction of the discovery of VdB0 that were reported in a previous version of the paper. We are grateful to M. Gieles, V.D. Ivanov, N. Caldwell, and, in particular, to M. Messineo for useful discussions and suggestions.
Funders:
Funding AgencyGrant Number
Istituto Nazionale di Astrofisica (INAF)CRA 1.06.10.04
Natural Sciences and Engineering Research Council of Canada (NSERC)UNSPECIFIED
NASAHST-GO-10818.01-A
National Research Council of CanadaUNSPECIFIED
NASA Hubble FellowshipUNSPECIFIED
Subject Keywords:galaxies: star clusters; galaxies: individual: M 31; supergiants; stars: evolution
Record Number:CaltechAUTHORS:20100413-105838778
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20100413-105838778
Official Citation:An HST/WFPC2 survey of bright young clusters in M 31 - IV. Age and mass estimates S. Perina, J. G. Cohen, P. Barmby, M. A. Beasley, M. Bellazzini, J. P. Brodie, L. Federici, F. Fusi Pecci, S. Galleti, P. W. Hodge, J. P. Huchra, M. Kissler-Patig, T. H. Puzia and J. Strader A&A 511 A23 (2010) DOI: 10.1051/0004-6361/200913459
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:17957
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:13 Apr 2010 21:39
Last Modified:10 Dec 2019 22:32

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