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Related papers: Internal dynamics and membership of the NGC 3603 Y…

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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…

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 aim to identify the cluster members, estimate cluster properties, study the dynamical state of the clusters as a function of mass, trace the existence of dynamical effects in massive stars, and check for spatial patterns of members in…

Solar and Stellar Astrophysics · Physics 2025-10-21 Harsha K. H. , Annapurni Subramaniam , S. R. Dhanush , Hariharan D. S

Based on deep VLT/ISAAC JHK photometry, we have derived the present-day mass function of the central starburst cluster NGC 3603 YC (Young Cluster) in the giant HII region NGC 3603. The effects of field contamination, individual reddening,…

Astrophysics · Physics 2008-11-26 Andrea Stolte , Wolfgang Brandner , Bernhard Brandl , Hans Zinnecker

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

We present a new method to determine the age spread of resolved stellar populations in a starburst cluster. The method relies on a two-step process. In the first step, kinematic members of the cluster are identified based on multi-epoch…

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 investigate the star cluster population in the outer parts of the starburst galaxy NGC 5253 using archive images taken with the Hubble Space Telescope's Advanced Camera for Surveys. Based on the F415W, F555W, and F814W photometry ages…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 D. Harbeck , J. Gallagher , D. Crnojević

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

By studying young open clusters, the mechanisms important for star formation over several Myr can be examined. For example, accretion rate as a function of rotational velocity can be investigated. Similarly, sequential star formation…

Astrophysics · Physics 2009-01-06 E. Paunzen , M. Netopil , K. Zwintz

We have obtained optical and near-infrared spectra of candidate members of the star-forming clusters IC 348 and NGC 1333. We classify 100 and 42 candidates as new members of the clusters, respectively, which brings the total numbers of…

Solar and Stellar Astrophysics · Physics 2016-08-17 K. L. Luhman , T. L. Esplin , N. P. Loutrel

The very bright and compact massive young cluster, NGC 3603, has been cited as an example of a starburst in the Milky Way and compared with the much-studied R136/30 Doradus region in the Large Magellanic Cloud. Here we build on the…

Solar and Stellar Astrophysics · Physics 2019-04-10 J. E. Drew , M. Monguió , N. J. Wright

We present a study of the young population in the starburst galaxy NGC 253. In particular, we focused our attention on searching young star groups, obtaining their main properties and studying their hierarchical organization. For this task,…

Astrophysics of Galaxies · Physics 2018-07-18 M. J. Rodríguez , G. Baume , C. Feinstein

We present high-resolution near-infrared imaging obtained using adaptive optics and HST/NICMOS, and ground-based spectroscopy of the hot-spot galaxy NGC2903. Our near-infrared resolution imaging enables us to resolve the infrared hot spots…

Astrophysics · Physics 2009-10-31 A. Alonso-Herrero , S. D. Ryder , J. H. Knapen

Based on kinematic data observed for very young, massive clusters that appear to be in dynamical equilibrium, it has recently been argued that such young systems set examples where the early residual gas-expulsion did not happen or had no…

Astrophysics of Galaxies · Physics 2015-06-12 Sambaran Banerjee , Pavel Kroupa

We have observed NGC 3603, the most massive visible HII region known in the Galaxy, with ANTU(VLT1)/ISAAC in the near-infrared (NIR) J_s, H, and K_s bands. Our observations are the most sensitive observations made to date of this dense…

Astrophysics · Physics 2007-05-23 B. Brandl , W. Brandner , F. Eisenhauer , A. F. J. Moffat , F. Palla , H. Zinnecker

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 a detailed clustering analysis of the young stellar population across the star-forming ring galaxy NGC 6503, based on the deep HST photometry obtained with the Legacy ExtraGalactic UV Survey (LEGUS). We apply a contour-based map…

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

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
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