643 citations · 2.7k across the 47 of their papers we have counts for
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astro-ph2003★ 156 cited
The dynamical mass of the young cluster W3 in NGC 7252: Heavy-Weight globular cluster or ultra compact dwarf galaxy ?
C. Maraston, N. Bastian, R. P. Saglia +3
We have determined the dynamical mass of the most luminous stellar cluster known to date, i.e. object W3 in the merger remnant galaxy NGC 7252. The dynamical mass is estimated from…
astro-ph2003★ 62 cited
A Variable Ultraluminous Supersoft X-ray Source in "The Antennae": Stellar-Mass Black Hole or White Dwarf?
G. Fabbiano, A. R. King, A. Zezas +3
The chandra monitoring observations of The Antennae (NGC 4038/39) have led to the discovery of a variable, luminous, supersoft source (SSS). This source is only detected at energie…