| タイトル | Fermi LAT Pulsed Detection of PSR J0737-3039A in the Double Pulsar System |
| 本文（外部サイト） | http://hdl.handle.net/2060/20140010707 |
| 著者（英） | Kramer, M.; Kerr, M.; Harding, A. K.; Romani, R. W.; Venter, C.; Ferdman, R. D.; Johnson, T. J.; Stairs, I. H.; Craig, H. A.; Guillemot, L. |
| 著者所属（英） | NASA Goddard Space Flight Center |
| 発行日 | 2013-05-10 |
| 言語 | eng |
| 内容記述 | We report the Fermi Large Area Telescope discovery of gamma-ray pulsations from the 22.7 ms pulsar A in the double pulsar system J07373039A/B. This is the first mildly recycled millisecond pulsar (MSP) detected in the GeV domain. The 2.7 s companion object PSR J07373039B is not detected in gamma rays. PSR J07373039A is a faint gamma-ray emitter, so that its spectral properties are only weakly constrained; however, its measured efficiency is typical of other MSPs. The two peaks of the gamma-ray light curve are separated by roughly half a rotation and are well offset from the radio and X-ray emission, suggesting that the GeV radiation originates in a distinct part of the magnetosphere from the other types of emission. From the modeling of the radio and the gamma-ray emission profiles and the analysis of radio polarization data, we constrain the magnetic inclination alpha and the viewing angle zeta to be close to 90 deg., which is consistent with independent studies of the radio emission from PSR J07373039A. A small misalignment angle between the pulsar's spin axis and the system's orbital axis is therefore favored, supporting the hypothesis that pulsar B was formed in a nearly symmetric supernova explosion as has been discussed in the literature already. |
| NASA分類 | Astronomy |
| レポートNO | GSFC-E-DAA-TN11222 |
| 権利 | Copyright, Distribution as joint owner in the copyright |
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