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We present multicolor photometry of bright star cluster candidates in the nearby starburst galaxies NGC 3077 and NGC 5253, observed with the Hubble Space Telescope Wide Field and Planetary Camera 2 in both broadband (F300W, F547M and F814W)…

Astrophysics · Physics 2009-11-10 J. Harris , D. Calzetti , J. S. Gallagher , D. A. Smith , C. J. Conselice

Using high-resolution Hubble Space Telescope data, we reexamine the fundamental properties (ages, masses and extinction values) of the rich star cluster population in the dwarf starburst galaxy NGC 5253. The gain in resolution compared to…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-15 Richard de Grijs , Peter Anders , Erik Zackrisson , Göran Östlin

We present a detailed analysis of the star cluster population in the starburst galaxy NGC 5253. Our work is based on HST optical and VLT Ks images. We detect more than 300 clusters, and for all of them we derive the photometry in the V, I…

Astrophysics · Physics 2009-11-10 G. Cresci , L. Vanzi , M. Sauvage

We present observations of a massive star cluster near the nuclear region of the nearby starburst galaxy NGC 253. The peak of near-infrared emission, which is spatially separated by 4" from the kinematic center of the galaxy, is coincident…

Solar and Stellar Astrophysics · Physics 2010-01-15 Katherine A. Kornei , Nate McCrady

Ultraviolet, optical and near infrared images of the nearby (D ~ 5.5 Mpc) SBm galaxy NGC 1311, obtained with the Hubble Space Telescope, reveal a small population of 13 candidate star clusters. We identify candidate star clusters based on a…

We investigate the star cluster system in the starburst galaxy NGC 7673 using archival Hubble Space Telescope WFPC2 broad-band images. For the first time we are able to examine the internal structures of the prominent optical clumps in this…

Astrophysics · Physics 2009-11-07 Nicole Homeier , John S. Gallagher , Anna Pasquali

We present a photometric catalog of 45 massive star clusters in the nuclear starburst of M 83 (NGC 5236), observed with the Hubble Space Telescope WFPC2, in both broad-band (F300W, F547M, and F814W) and narrow-band (F656N and F487N)…

Astrophysics · Physics 2009-11-07 J. Harris , D. Calzetti , J. S. Gallagher , C. J. Conselice , D. A. Smith

The nearby dwarf starburst galaxy NGC5253 hosts a number of young, massive star clusters, the two youngest of which are centrally concentrated and surrounded by thermal radio emission (the `radio nebula'). To investigate the role of these…

We present new observations of the famous starburst galaxy NGC 5253 which owes its celebrity to possibly being the youngest and closest starburst galaxy known. Our observations in the infrared and millimeter contribute to shed light on the…

Astrophysics · Physics 2016-08-30 Leonardo Vanzi , Marc Sauvage

The blue compact dwarf galaxy NGC 5253 hosts a very young starburst containing twin nuclear star clusters, separated by a projected distance of 5 pc. One cluster (#5) coincides with the peak of the H-alpha emission and the other (#11) with…

Astrophysics of Galaxies · Physics 2016-06-01 L. J. Smith , P. A. Crowther , D. Calzetti , F. Sidoli

The blue compact dwarf galaxy NGC 5253 hosts a very young central starburst. The center contains intense radio thermal emission from a massive ultracompact H II region (or "supernebula") and two massive and very young super star clusters…

Astrophysics of Galaxies · Physics 2020-06-24 Linda J. Smith , Varun Bajaj , Jenna Ryon , Elena Sabbi

The intermediate age star cluster W3 (age ~ 300-500 Myr) in NGC 7252 is the most luminous star cluster known to date with a dynamical mass estimate of 8 +/- 2 x 10^7 M_sun. With an effective radius of about 17.5 pc and a velocity dispersion…

Astrophysics · Physics 2009-11-10 M. Fellhauer , P. Kroupa

NGC 253 hosts the nearest nuclear starburst. Previous observations show a region rich in molecular gas, with dense clouds associated with recent star formation. We used ALMA to image the 350 GHz dust continuum and molecular line emission…

Hidden from optical view in the starburst region of the dwarf galaxy NGC 5253 lies an intense radio source with an unusual spectrum which could be interpreted variously as nebular gas ionized by a young stellar cluster or nonthermal…

Astrophysics · Physics 2009-11-06 Varoujan Gorjian , Jean L. Turner , Sara C. Beck

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…

Astrophysics of Galaxies · Physics 2015-06-17 A. Sollima , M. Cignoni , R. G. Gratton , M. Tosi , A. Bragaglia , S. Lucatello , G. Meurer

The young star cluster W3 (age 300-500 Myr) in NGC 7252 is the most luminous star cluster known to date. Dynamical mass estimates result in 8 +/- 2 * 10^7 M_sun. With an effective radius of about 18 pc and a velocity dispersion of 45 km/s…

Astrophysics · Physics 2007-05-23 M. Fellhauer , P. Kroupa

We have used new, deep, visible and near infrared observations of the compact starburst cluster in the giant HII region NGC 3603 and its surroundings with the WFC3 on HST and HAWK-I on the VLT to study in detail the physical properties of…

A local dwarf galaxy, NGC 5253, has a young super star cluster that may provide an example of highly efficient star formation. Here we report the detection and imaging, with the Submillimeter Array, of the J= 3-2 rotational transition of CO…

Astrophysics of Galaxies · Physics 2015-03-19 J. L. Turner , S. C. Beck , D. J. Benford , S. M. Consiglio , P. T. P. Ho , A. Kovács , D. S. Meier , J. -H. Zhao

Early release science observations of the cluster NGC3603 with the WFC3 on the refurbished HST allow us to study its recent star formation history. Our analysis focuses on stars with Halpha excess emission, a robust indicator of their…

We have collected archival data on NGC7673 to constrain the star-formation history that produced the young star clusters and the field stellar population in this galaxy during the last 2 Gyr. We have considered the sample of 50 star…

Astrophysics · Physics 2009-11-13 A. Pasquali , P. Castangia
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