E.P.J. van den Heuvel
University of Amsterdam
236 Papers
2.8K Citations
E.P.J. van den Heuvel is an academic researcher from University of Amsterdam. The author has contributed to research in topics: Neutron star & Pulsar. The author has an hindex of 60, co-authored 236 publications. Previous affiliations of E.P.J. van den Heuvel include European Southern Observatory & Kavli Institute for Theoretical Physics.
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Papers
•Journal Article
The formation of close-binary systems in globular clusters.
TL;DR: In this article, the formation continue de systemes binaires serres dans les amas globulaires par collision and capture, and the fonction de masse initiale moyenne de tous les amaars globuleaires doit etre plus aigue qu'une loi de puissance d'indice −3
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Physics of the GRB 030328 afterglow and its environment
E. Maiorano,E. Maiorano,N. Masetti,Eliana Palazzi,Sandra Savaglio,Evert Rol,Paul Vreeswijk,Elena Pian,Paul A. Price,Paul A. Price,Bruce A. Peterson,Martin Jelínek,Lorenzo Amati,Michael I. Andersen,A. J. Castro-Tirado,J. M. Castro Cerón,A. de Ugarte Postigo,F. Frontera,F. Frontera,A. S. Fruchter,Johan P. U. Fynbo,Javier Gorosabel,Arne Henden,Jens Hjorth,B. L. Jensen,Sylvio Klose,Chryssa Kouveliotou,Gianluca Masi,Palle Møller,Luciano Nicastro,Eran O. Ofek,Shashi B. Pandey,Shashi B. Pandey,James E. Rhoads,Nial R. Tanvir,Ralph A. M. J. Wijers,E.P.J. van den Heuvel +36 more
TL;DR: In this article, the optical afterglow of Gamma-Ray Burst (GRB) 030328 detected by HETE-2 was monitored using photometric, spectroscopic and polarimetric methods.
Forty Years of X-Ray Binaries
E.P.J. van den Heuvel
- 17 Jun 2014
TL;DR: In this article, the formation rate, duration of the X-ray phase and later evolution after the Xray phase of the HMXBs are discussed, and the causes of these long periods and of the outbursts of SFXTs are discussed.
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The optical/near-IR spectral energy distribution of the GRB 000210 host galaxy
J. Gorosabel,Lise Christensen,Jens Hjorth,J. P. U. Fynbo,Henrik D. Pedersen,B. L. Jensen,Marilyne Andersen,Niels Lund,Andreas O. Jaunsen,J. M. Castro Cerón,A. J. Castro-Tirado,A. S. Fruchter,Jochen Greiner,Elena Pian,P. M. Vreeswijk,I. Burud,F. Frontera,L. Kaper,S. Klose,Chryssa Kouveliotou,N. Masetti,Eliana Palazzi,James E. Rhoads,E. Rol,I. Salamanca,Nial R. Tanvir,Ralph A. M. J. Wijers,E.P.J. van den Heuvel +27 more
- 01 Jun 2004
TL;DR: In this article, a grid of spectral templates were used to fit the SED of the dark GRB 000210 host galaxy to its Spectral Energy Distribution (SED) and derived a photometric redshift (z=0.842\+0.0540) which is in excellent agreement with the spectroscopic one (z = 0.8463+/-0.0002).
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