G. Nelemans
Radboud University Nijmegen
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Publication
Featured researches published by G. Nelemans.
Physical Review Letters | 2017
B. Abbott; S. Bloemen; P. Canizares; S. Ghosh; P. Groot; T. Hinderer; G. Nelemans; D. Nichols; S. Nissanke; P. Schmidt; A.R. Williamson
On August 17, 2017 at 12:41:04 UTC the Advanced LIGO and Advanced Virgo gravitational-wave detectors made their first observation of a binary neutron star inspiral. The signal, GW170817, was detected with a combined signal-to-noise ratio of 32.4 and a false-alarm-rate estimate of less than one per
Astronomy and Astrophysics | 2001
G. Nelemans; Lev R. Yungelson; S. Portegies Zwart; F. Verbunt
8.0\times10^4
Astronomy and Astrophysics | 2001
G. Nelemans; S. Portegies Zwart; F. Verbunt; Lev R. Yungelson
years. We infer the component masses of the binary to be between 0.86 and 2.26
Astronomy and Astrophysics | 2001
G. Nelemans; Lev R. Yungelson; S. Portegies Zwart
M_\odot
Astronomy and Astrophysics | 2006
J. P. U. Fynbo; Rhaana L. C. Starling; Cedric Ledoux; Klaas Wiersema; C. C. Thöne; Jesper Sollerman; P. Jakobsson; J. Hjorth; D. Watson; Paul M. Vreeswijk; P. Møller; E. Rol; J. Gorosabel; Jyri Naranen; R. A. M. J. Wijers; G. Björnsson; J. M. Castro Cerón; P. A. Curran; Dieter H. Hartmann; Stephen T. Holland; B. L. Jensen; Andrew J. Levan; Marceau Limousin; C. Kouveliotou; G. Nelemans; Robert S. Priddey; Nial R. Tanvir
, in agreement with masses of known neutron stars. Restricting the component spins to the range inferred in binary neutron stars, we find the component masses to be in the range 1.17 to 1.60
The Astrophysical Journal | 2009
J. C. A. Miller-Jones; P. G. Jonker; V. Dhawan; W. Brisken; Michael P. Rupen; G. Nelemans; Elena Gallo
M_\odot
Astrophysical Journal Supplement Series | 2011
P. G. Jonker; C. G. Bassa; G. Nelemans; D. Steeghs; M. A. P. Torres; Thomas J. Maccarone; Robert I. Hynes; James L. Clem; A. Dieball; V. Mikles; C. T. Britt; L. Gossen; A. Collazzi; Rudy Wijnands; J. in't Zand; Mariano Mendez; N. Rea; E. Kuulkers; E. M. Ratti; L.M. van Haaften; Craig O. Heinke; Feryal Ozel; P. Groot; F. Verbunt
, with the total mass of the system
Astronomy and Astrophysics | 2007
M. Vučković; Conny Aerts; Roy Ostensen; G. Nelemans; Haili Hu; C. S. Jeffery; V. S. Dhillon; T. R. Marsh
2.74^{+0.04}_{-0.01}\,M_\odot
The Astrophysical Journal | 2008
R. Wesson; Michael J. Barlow; Romano L. M. Corradi; Janet E. Drew; P. Groot; Christian Knigge; D. Steeghs; Boris T. Gaensicke; R. Napiwotzki; P. Rodríguez-Gil; Albert A. Zijlstra; M. F. Bode; Jeremy J. Drake; David J. Frew; E. Gonzalez-Solares; R. Greimel; M. J. Irwin; L. Morales-Rueda; G. Nelemans; Quentin A. Parker; S. E. Sale; Jennifer Lynn Sokoloski; A. Somero; Helena Uthas; N. A. Walton; Brian Warner; C. A. Watson; N. J. Wright
. The source was localized within a sky region of 28 deg
Astronomy and Astrophysics | 2005
D.J. Lommen; L. Yungelson; van den Heuvel; G. Nelemans; S. Portegies Zwart
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