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| Query : 1997A&A...317L..87U |
1997A&A...317L..87U - Astronomy and Astrophysics, volume 317, L87-90 (1997/1-3)
On the persistent X-ray emission from the soft γ-ray repeaters.
USOV V.V.
Abstract (from CDS):
It is suggested that the persistent X-ray emission from the soft γ-ray repeaters is the thermal radiation of neutron stars which are enhanced by a factor of 10 or more due to the effect of a very strong magnetic field on the thermal structure of the neutron star envelope. For the thermal luminosity to be consistent with the persistent X-ray luminosity, the field strength at the neutron star surface has to be of the order of 1015G. If it is confirmed that the soft γ-ray repeaters are neutron stars with negligible accretion, then the presence of such a strong magnetic field is inevitable.
Abstract Copyright: ∼
Journal keyword(s): gamma-rays: bursters - stars: neutron - magnetic fields - radiation mechanisms: thermal
Simbad objects: 6
| Number of rows : 6 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2024 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | SNR J052559-660453 | SNR | 05 26 00.4 | -66 05 02 | 12.71 | ~ | 437 | 2 | ||||
| 2 | PSR B0525-66 | Psr | 05 26 00.7 | -66 04 35 | ~ | 545 | 1 | |||||
| 3 | AX J1808.6-2024 | ISM | 18 08 39 | -20 24.6 | ~ | 130 | 3 | |||||
| 4 | PSR J1808-2024 | Psr | 18 08 39.32 | -20 24 40.1 | ~ | 1240 | 2 | |||||
| 5 | GBS 1900+14 | gB | 19 07 13 | +09 19.6 | ~ | 857 | 0 | |||||
| 6 | SNR G042.8+00.6 | SNR | 19 07 41.9 | +09 07 17 | ~ | 129 | 1 |
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