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20042026
most citedThe Age Distribution of Massive Star Clusters in the Antennae Galaxies

243 citations · 6.4k across the 138 of their papers we have counts for

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Showing 2012Show all

6 papers · 1 filter

astro-ph.CO2012★ 19 cited

X-ray Binaries and Star Clusters in the Antennae: Optical Cluster Counterparts

Blagoy Rangelov, Rupali Chandar, Andrea Prestwich +1

We compare the locations of 82 X-ray binaries (XRBs) detected in the merging Antennae galaxies by Zezas et al., based on observations taken with the Chandra X-Ray Observatory, with…

astro-ph.GA2012★ 29 cited

Evidence for Two Distinct Stellar Initial Mass Functions

Dennis Zaritsky, Janet E. Colucci, Peter M. Pessev +2

We present velocity dispersion measurements of 20 Local Group stellar clusters (7 < log(age [yrs]) < 10.2) from integrated light spectra and examine the evolution of the stellar ma…

astro-ph.GA2012

Space-Based UV/Optical Wide-Field Imaging and Spectroscopy: Near-Field Cosmology and Galaxy Evolution Using Globular Clusters in Nearby Galaxies

Paul Goudfrooij, Jean Brodie, Rupali Chandar +7

Star formation plays a central role in the evolution of galaxies and of the Universe as a whole. Studies of star-forming regions in the local universe have shown that star formatio…

astro-ph.GA2012★ 112 cited

Similarities in Populations of Star Clusters

S. Michael Fall, Rupali Chandar

We compare the observed mass functions and age distributions of star clusters in six well-studied galaxies: the Milky Way, Magellanic Clouds, M83, M51, and Antennae. In combination…

astro-ph.GA2012★ 26 cited

The Resolved Stellar Population in 50 Regions of M83 from HST/WFC3 Early Release Science Observations

Hwihyun Kim, Bradley C. Whitmore, Rupali Chandar +22

We present a multi-wavelength photometric study of ~15,000 resolved stars in the nearby spiral galaxy M83 (NGC5236, D=4.61Mpc) based on Hubble Space Telescope Wide Field Camera 3 o…

astro-ph.CO2012★ 68 cited

Analysing star cluster populations with stochastic models: the HST/WFC3 sample of clusters in M83

Morgan Fouesneau, Ariane Lançon, Rupali Chandar +1

The majority of clusters in the Universe have masses well below 10^5 Msun. Hence their integrated fluxes and colors can be affected by the random presence of a few bright stars int…