astro-ph.HE : High Energy Astrophysical Phenomena
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Monday, September 3, 2012
1208.6292 (S. Scaringi et al.)
Broad-band timing properties of the accreting white dwarf MV Lyrae
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S. Scaringi, E. Koerding, P. Uttley, P. J. Groot, C. Knigge, M. Still, P. Jonker
1208.6364 (Rahul Basu et al.)
On the nature of Off-pulse emission from pulsars
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Rahul Basu, Dipanjan Mitra, Ramana Athreya
1208.6400 (Karabi Ghosh)
Analytical benchmark for the non-equilibrium Marshak diffusion problem in a planar slab of finite thickness
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Karabi Ghosh
1208.6437 (L. Zaninetti)
Evolution of superbubbles in a self-gravitating disk
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L. Zaninetti
1208.6443 (Michael Gabler et al.)
Magneto-elastic oscillations of neutron stars II: exploring different magnetic field configurations
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Michael Gabler, Pablo Cerdá-Durán, José A. Font, Ewald Müller, Nikolaos Stergioulas
1208.6446 (Silvia Toonen et al.)
Supernova Type Ia progenitors from merging double white dwarfs: Using a new population synthesis model
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Silvia Toonen, Gijs Nelemans, Simon Portegies Zwart
1208.6470 (S. A. Petrova)
Axisymmetric force-free magnetosphere of a pulsar. I. The structure close to the magnetic axis
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S. A. Petrova
1208.6511 (J. Lopez-Santiago et al.)
AE Aurigae: first detection of non-thermal X-ray emission from a bow shock produced by a runaway star
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J. Lopez-Santiago, M. Miceli, M. V. del Valle, G. E. Romero, R. Bonito, J. F. Albacete-Colombo, V. Pereira, E. de Castro, F. Damiani
1208.6522 (Neil Gehrels et al.)
Gamma Ray Bursts
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Neil Gehrels, Peter Meszaros
1208.6574 (Mariangela Settimo et al.)
Measurement of the cosmic ray energy spectrum using hybrid events of the Pierre Auger Observatory
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Mariangela Settimo, for the Pierre Auger Collaboration
1208.6576 (D. R. Lorimer et al.)
Radio and X-ray observations of the intermittent pulsar J1832+0029
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D. R. Lorimer, A. G. Lyne, M. A. McLaughlin, G. G. Pavlov, C. Chang
1208.6582 (A. Y. Potekhin et al.)
Radiative properties of magnetic neutron stars with metallic surfaces and thin atmospheres
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A. Y. Potekhin, V. F. Suleimanov, M. van Adelsberg, K. Werner
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