activity
20062015
most citedGas expulsion and the destruction of massive young clusters

392 citations · 796 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2015★ 9 cited

A Comprehensive HST BVI Catalogue Of Star Clusters In Five Hickson Compact Groups Of Galaxies

K. Fedotov, S. C. Gallagher, P. R. Durrell +5

We present a photometric catalogue of star cluster candidates in Hickson compact groups (HCGs) 7, 31, 42, 59, and 92, based on observations with the Advanced Camera for Surveys and…

astro-ph.SR2011★ 106 cited

The VLT-FLAMES Tarantula Survey III: A very massive star in apparent isolation from the massive cluster R136

Joachim M. Bestenlehner, Jorick S. Vink, G. Gräfener +17

VFTS 682 is located in an active star-forming region, at a projected distance of 29 pc from the young massive cluster R136 in the Tarantula Nebula of the Large Magellanic Cloud. It…

astro-ph.SR2011★ 287 cited

The VLT-FLAMES Tarantula Survey I: Introduction and observational overview

C. J. Evans, W. D. Taylor, V. Henault-Brunet +39

The VLT-FLAMES Tarantula Survey (VFTS) is an ESO Large Programme that has obtained multi-epoch optical spectroscopy of over 800 massive stars in the 30 Doradus region of the Large…

astro-ph.CO2011

The FLAMES Tarantula Survey

N. Markova, C. Evans, N. Bastian +30

The Tarantula survey is an ESO Large Programme which has obtained multi-epochs spectroscopy of over 800 massive stars in the 30 Dor region in the Large Magelanic Cloud. Here we bri…

astro-ph2008★ 1 cited

New Results on the Ages of Star Clusters in Region B of M82

I. S. Konstantopoulos, N. Bastian, L. J. Smith +3

The post-starburst region B in M82 and its massive star cluster component have been the focus of multiple studies, with reports that there is a large population of coeval clusters…

astro-ph2006★ 392 cited

Gas expulsion and the destruction of massive young clusters

Simon P. Goodwin, Nate Bastian

We examine the luminosity and dynamical mass estimates for young massive stellar clusters. For many young (<50 Myr) clusters, the luminosity and dynamical mass estimates differ by…