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相关论文: Effective Radii of Young, Massive Star Clusters in…

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We measure the projected half-light radii of young star clusters in 31 galaxies from the Legacy Extragalactic UV Survey (LEGUS). We implement a custom pipeline specifically designed to be robust against contamination, which allows us to…

星系天体物理 · 物理学 2021-10-20 Gillen Brown , Oleg Y. Gnedin

We measure the radii and two-dimensional light profiles of a large sample of young, massive star clusters in M83 using archival HST/WFC3 imaging of seven adjacent fields. We use GALFIT to fit the two-dimensional light profiles of the…

We present a study of the spatial distribution of the stellar cluster populations in the star forming galaxy NGC 628. Using Hubble Space Telescope broad band WFC3/UVIS UV and optical images from the Treasury Program LEGUS (Legacy…

We examine the spatial distribution of star clusters in NGC 628 using the statistical tool INDICATE to quantify clustering tendencies. Our sample, based on HST and JWST observations, is the most complete to date, spanning ages from 1 Myr to…

We obtained Hubble Space Telescope/Wide Field Camera 3 imaging of a sample of ten of the nearest and brightest nuclear clusters residing in late-type spiral galaxies, in seven bands that span the near-ultraviolet to the near-infrared.…

We exploit the superb resolution of the new HST/ACS mosaic image of M51 to select a large sample of young (< 1 Gyr) star clusters in the spiral disk, based on their sizes. The image covers the entire spiral disk in B, V, I and H_alpha, at a…

天体物理学 · 物理学 2015-06-24 R. A. Scheepmaker , M. Gieles , M. R. Haas , N. Bastian , S. S. Larsen , H. J. G. L. M. Lamers

We present Hubble Space Telescope (HST) Wide-Field Camera 3 (WFC3) images of the merger remnant NGC 7252. In particular, we focus on the surface brightness profiles and effective radii, Reff, of 36 young massive clusters (YMCs) within the…

宇宙学与河外天体物理 · 物理学 2015-06-12 Nate Bastian , Francois Schweizer , Paul Goudfrooij , Soeren S. Larsen , Markus Kissler-Patig

(abridged) We present a comprehensive study of stellar stratification in young star clusters in the Large Magellanic Cloud (LMC). We apply our recently developed effective radius method for the assessment of stellar stratification on…

星系天体物理 · 物理学 2015-05-14 Dimitrios A. Gouliermis , Dougal Mackey , Yu Xin , Boyke Rochau

A detailed description is given of the data analysis leading to the discovery of young massive star clusters (YMCs) in a sample of 21 nearby galaxies. A new useful tool, ishape, for the derivation of intrinsic shape parameters of compact…

天体物理学 · 物理学 2009-10-31 S. S. Larsen

We present a new catalog and results for the cluster system of the starburst galaxy NGC 4449 based on multi-band imaging observations taken as part of the LEGUS and Halpha-LEGUS surveys. We improve the spectral energy fitting method used to…

Using ground-based UBVRI+Halpha CCD photometry we have been carrying out a search for young massive star clusters (YMCs) in a sample consisting of 21 nearby spiral galaxies. We find a large variety concerning the richness of the cluster…

天体物理学 · 物理学 2007-05-23 Soeren S. Larsen , Tom Richtler

In the lenticular galaxy NGC 1023 a new population of star clusters (``faint fuzzies'') was recently discovered by Larsen & Brodie. These clusters are found inside the disc and are faint (23 < V < 24 mag) and extended with effective radii…

天体物理学 · 物理学 2009-11-07 M. Fellhauer , P. Kroupa

In this work we improve a previously published method to calculate in a reliable way the radius of an open cluster. The method is based on the behaviour of stars in the proper motion space as the sampling changes in the position space. Here…

星系天体物理 · 物理学 2020-05-27 Nestor Sanchez , Emilio Alfaro , Fatima Lopez-Martinez

We investigate the structural properties of nuclear star clusters in late-type spiral galaxies. More specifically, we fit analytical models to HST images of 39 nuclear clusters in order to determine their effective radii after correction…

天体物理学 · 物理学 2009-11-10 T. Boeker , M. Sarzi , D. E. McLaughlin , R. P. van der Marel , H. -W. Rix , L. C. Ho , J. C. Shields

Using Magellan/IMACS images covering a 1.2 x 1.2 sq. degree FOV with seeing of 0.4"-0.6", we have applied convolution techniques to analyse the light distribution of 364 confirmed globular cluster in the field of NGC 5128 and to obtain…

天体物理学 · 物理学 2009-11-13 M. Gomez , K. A. Woodley

We present the results of deep high resolution imaging performed with ACS/HRC@HST in the most active region of the nearby starburst galaxy NGC 4214. We resolved the stellar populations of five Young Massive Clusters and their surrounding…

星系天体物理 · 物理学 2015-06-17 A. Sollima , M. Cignoni , R. G. Gratton , M. Tosi , A. Bragaglia , S. Lucatello , G. Meurer

The young cluster NGC 6231 (stellar ages ~2-7 Myr) is observed shortly after star-formation activity has ceased. Using the catalog of 2148 probable cluster members obtained from Chandra, VVV, and optical surveys (Paper I), we examine the…

HST WFPC1 observations revealed 738 bright star clusters spread over the inner 12 kpc of the interacting galaxy pair NGC 4038/39. If the young star clusters (YSCs) formed in the global starburst are (proto-) globular or open clusters has…

天体物理学 · 物理学 2007-05-23 Uta Fritze - v. Alvensleben , Oliver Kurth
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