| People | Locations | Statistics |
|---|---|---|
| Naji, M. |
| |
| Motta, Antonella |
| |
| Aletan, Dirar |
| |
| Mohamed, Tarek |
| |
| Ertürk, Emre |
| |
| Taccardi, Nicola |
| |
| Kononenko, Denys |
| |
| Petrov, R. H. | Madrid |
|
| Alshaaer, Mazen | Brussels |
|
| Bih, L. |
| |
| Casati, R. |
| |
| Muller, Hermance |
| |
| Kočí, Jan | Prague |
|
| Šuljagić, Marija |
| |
| Kalteremidou, Kalliopi-Artemi | Brussels |
|
| Azam, Siraj |
| |
| Ospanova, Alyiya |
| |
| Blanpain, Bart |
| |
| Ali, M. A. |
| |
| Popa, V. |
| |
| Rančić, M. |
| |
| Ollier, Nadège |
| |
| Azevedo, Nuno Monteiro |
| |
| Landes, Michael |
| |
| Rignanese, Gian-Marco |
|
Enoto, T.
in Cooperation with on an Cooperation-Score of 37%
Topics
Publications (8/8 displayed)
- 2016Measurements of the Soft Gamma-Ray Emission from SN2014J with Suzakucitations
- 2010Wide-band Suzaku Analysis of the Persistent Emission from SGR 0501+4516 During the 2008 Outburstcitations
- 2009Suzaku Observation of the New Soft Gamma Repeater SGR 0501+4516 in Outburstcitations
- 2008Possible Suzaku detection of non-thermal X-ray signals from a rotating magnetized white dwarfcitations
- 2007Suzaku observations of cyclotron resonances in binary X-ray pulsarscitations
- 2006Possible Suzaku detection of non-thermal X-ray signals from a rotating magnetized white dwarf
- 2006Possible Suzaku detection of non-thermal X-ray signals from a rotating magnetized white dwarf
- 2006Possible Suzaku detection of non-thermal X-ray signals from a rotating magnetized white dwarf
Places of action
| Organizations | Location | People |
|---|
article
Possible Suzaku detection of non-thermal X-ray signals from a rotating magnetized white dwarf
Abstract
Although rotating neutron stars (NSs) have been regarded as being textbook examples of astrophysical particle acceleration sites for decades, details of the acceleration mechanism remain a mystery; for example, we cannot yet observationally distinguish “polar cap” models from “outer gap” models. To solve the model degeneracy, it is useful to study similar systems with much different physical parameters. Strongly magnetized white dwarfs (WDs) are ideal for this purpose, because they have essentially the same system geometry as NSs, but differ largely from NSs in the system parameters, including the size, magnetic field, and the rotation velocity, with the induced electric field expected to reach 10<SUP>13</SUP> 10<SUP>14</SUP> eV. Based on this idea, the best candidate among WDs, AE Aquarii, was observed with the fifth Japaneses X-ray satellite, Suzaku. The hard X-ray detector (HXD) on-board Suzaku has the highest sensitivity in the hard X-ray band over 10 keV. A marginal detection in the hard X-ray band was achieved with the HXD, and was separated from the thermal emission. The flux corresponds to about 0.02% of its spin-down energy. If the signal is real, this observation must be a first case of the detection of non-thermal emission from WDs....