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相关论文: An HST/WFPC2 Survey of Bright Young Clusters in M3…

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We present an updated catalog of 1300 objects in the field of M31, including 670 likely star clusters of various types. Archival images were inspected to confirm cluster classifications where possible, but most of the classifications were…

We report on the properties of 89 low mass star clusters located in the vicinity of luminous young clusters (blue globulars) in the disk of M31. 82 of the clusters are newly detected. We have determined their integrated magnitudes and…

星系天体物理 · 物理学 2015-05-13 P. W. Hodge , O. K. Krienke , M. Bellazzini , S. Perina , P. Barmby , J. G. Cohen , T. H. Puzia , J. Strader

{Aims.} We present the main results of an imaging survey of possible young massive clusters (YMC) in M31 performed with the Wide Field and Planetary Camera2 (WFPC2) on the Hubble Space Telescope (HST). We present the images and color…

We have carried out a survey of compact star clusters (apparent size <3 arcsec) in the southwest part of the M31 galaxy, based on the high-resolution Suprime-Cam images (17.5 arcmin x 28.5 arcmin), covering ~15% of the deprojected galaxy…

星系天体物理 · 物理学 2009-11-18 V. Vansevicius , K. Kodaira , D. Narbutis , R. Stonkute , A. Bridzius , V. Deveikis , D. Semionov

In our study of M31's globular cluster system with MMT/Hectospec, we have obtained high-quality spectra of 85 clusters with ages less than 1 Gyr. With the exception of Hubble V, the young cluster in NGC 205, we find that these young…

We present the morphological properties of 161 star clusters in M33 using the Advanced Camera For Surveys Wide Field Channel onboard the Hubble Space Telescope using observations with the F606W and F814W filters. We obtain, for the first…

星系天体物理 · 物理学 2015-06-05 Izaskun San Roman , Ata Sarajedini , Jon A. Holtzman , Donald R. Garnett

We present a method for finding clusters of young stars in M31 using broadband WFPC2 data from the HST data archive. Applying our identification method to 13 WFPC2 fields, covering an area of ~60 arcmin^2, has revealed 79 new candidate…

天体物理学 · 物理学 2009-11-06 Benjamin F. Williams , Paul W. Hodge

The structures of globular clusters (GCs) reflect their dynamical states and past histories. High-resolution imaging allows the exploration of morphologies of clusters in other galaxies. Surface brightness profiles from new Hubble Space…

天体物理学 · 物理学 2009-06-23 P. Barmby , D. E. McLaughlin , W. E. Harris , G. L. H. Harris , D. A. Forbes

We present new high signal-to-noise spectroscopic data on the M31 globular cluster system, obtained with the Hectospec multifiber spectrograph on the 6.5m MMT. More than 300 clusters have been observed at a resolution of 5A. The primary…

星系天体物理 · 物理学 2015-05-27 Nelson Caldwell , Ricardo Schiavon , Heather Morrison , James A. Rose , Paul Harding

{Aims.} We introduce our imaging survey of possible young massive globular clusters in M31 performed with the Wide Field and Planetary Camera 2 (WFPC2) on the Hubble Space Telescope (HST). We present here details of the data reduction…

In this paper, we present surface brightness profiles for 79 globular clusters in M31, using images observed with {\it Hubble Space Telescope}, some of which are from new observations. The structural and dynamical parameters are derived…

宇宙学与河外天体物理 · 物理学 2015-06-15 Song Wang , Jun Ma

We present an updated UBVRI photometric catalog containing 970 objects in the field of M31, selected from the Revised Bologna Catalog (RBC v.4.0), including 965, 967, 965, 953, and 827 sources in the individual UBVRI bands, respectively, of…

宇宙学与河外天体物理 · 物理学 2015-05-20 Zhou Fan , Richard de Grijs , Xu Zhou

With the aim of increasing the sample of M31 clusters for which a colour magnitude diagram is available, we searched the HST archive for ACS images containing objects included in the Revised Bologna Catalogue of M31 globular clusters.…

宇宙学与河外天体物理 · 物理学 2015-05-14 Sibilla Perina , Luciana Federici , Michele Bellazzini , Carla Cacciari , Flavio Fusi Pecci , Silvia Galleti

This paper reports on a survey of star clusters in M31 based on archival images from the Hubble Space Telescope. Paper I (Krienke and Hodge 2007) reported results from images obtained with the Wide Field/Planetary Camera 2 (WFPC2) and this…

天体物理学 · 物理学 2007-11-29 O. K. Krienke , Paul W. Hodge

The ages and metallicities of globular clusters play an important role not just in testing models for their formation and evolution but in understanding the assembly history for their host galaxies. Here we use a combination of imaging and…

星系天体物理 · 物理学 2024-01-26 Christopher Usher , Nelson Caldwell , Ivan Cabrera-Ziri

We combine archival images for the nearby galaxy M33 (Triangulum Galaxy) from the ultraviolet (UV) to the infrared (IR) to derive ages, masses, and extinctions for the young star cluster population, and compare our physical parameters with…

星系天体物理 · 物理学 2021-12-22 Caitlin Moeller , Daniela Calzetti

In this paper, we present internal surface brightness profiles, using images in the F606W and F814W filter bands observed with the Advanced Camera for Surveys on the {\it Hubble Space Telescope}, for ten globular clusters (GCs) in the outer…

宇宙学与河外天体物理 · 物理学 2015-06-04 Song Wang , Jun Ma

We have studied the properties of a sample of 67 very blue and likely young massive clusters in M31 extracted from the Bologna Revised Catalog of globular clusters, selected according to their color [(B-V) < 0.45] and/or to the strength of…

天体物理学 · 物理学 2008-11-26 F. Fusi Pecci , M. Bellazzini , A. Buzzoni , E. De Simone , L. Federici , S. Galleti

In this paper, we present the properties of 10 halo globular clusters with luminosities $L\simeq 5-7\times 10^5{L_\odot}$ in the Local Group galaxy M33 using the images of {\it Hubble Space Telescope} Wide Field Planetary Camera 2 in the…

星系天体物理 · 物理学 2015-06-24 Jun Ma

The large majority of extragalactic star cluster studies performed to date essentially use multi-colour photometry, combined with theoretical stellar synthesis models, to derive ages, masses, extinction estimates, and metallicities. M31…

天体物理学 · 物理学 2009-11-11 Z. Fan , J. Ma , R. de Grijs , Y. Yang , X. Zhou
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