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19912026
most citedExperimental and Theoretical Challenges in the Search for the Quark Gluon Plasma: The STAR Collaboration's Critical Assessment of the Evidence from RHIC Collisions

3.4k citations

Showing 2003 · astro-phShow all

32 papers · 2 filters

astro-ph2003★ 6 cited

Two spectral states of the transient X-ray burster SAX J1747.0-2853

L. Natalucci, A. Bazzano, M. Cocchi +4

The neutron star binary SAX J1747.0-2853, located in the Galactic Center region at about 0.5 deg from Sgr A* and at a distance of 9 kpc, has been observed in outburst four times (1…

astro-ph2003

Magnetic field generation in relativistic shocks

Jorrit Wiersma, A. Achterberg

We present an analytical estimate for the magnetic field strength generated by the Weibel instability in ultra-relativistic shocks in a hydrogen plasma. We find that the Weibel ins…

astro-ph2003★ 52 cited

GBT Discovery of Two Binary Millisecond Pulsars in the Globular Cluster M30

Scott M. Ransom, Ingrid H. Stairs, Donald C. Backer +4

We report the discovery of two binary millisecond pulsars in the core-collapsed globular cluster M30 using the Green Bank Telescope (GBT) at 20 cm. PSR J2140-2310A (M30A) is an ecl…

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★ 45 cited

A Chandra observation of the old open cluster M67

Maureen van den Berg, Gianpiero Tagliaferri, Tomaso Belloni +1

We present the results of a 47-ks Chandra-ACIS observation of the old open cluster M67. We detected 25 proper-motion cluster members (including ten new sources) and 12 sources (all…

astro-ph2003★ 1 cited

Magnetic field decay, or just period-dependent beaming?

Joeri van Leeuwen, Frank Verbunt

Several recent papers conclude that radio-pulsar magnetic fields decay on a time-scale of 10 Myr, apparently contradicting earlier results. We have implemented the methods of these…