| タイトル | Gamma-ray burster counterparts - Radio |
| 著者（英） | Schaefer, Bradley E.; Evans, W. D.; Hurley, K.; Teegarden, B. J.; Fenimore, E. E.; Desai, U. D.; Estulin, I. V.; Atteia, J.-L.; Barat, C.; Cline, Thomas L. |
| 著者所属（英） | NASA Goddard Space Flight Center|Institute of Space Research|Centre d'Etude Spatiale des Rayonnements|California Univ.|Los Alamos National Lab.|Maryland Univ. |
| 発行日 | 1989-05-01 |
| 言語 | eng |
| 内容記述 | Many observers and theorists have suggested that gamma-ray bursters (GRBs) are related to highly magnetized rotating, neutron stars, in which case an analogy with pulsars implies that GRBs would be prodigious emitters of polarized radio emission during quiescence. The paper reports on a survey conducted with the Very Large Array radio telescope of 10 small GRB error regions for quiescent radio emission at wavelengths of 2, 6, and 20 cm. The sensitivity of the survey varied from 0.1 to 0.8 mJy. The observations did indeed reveal four radio sources inside the GRB error regions. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 89A37718 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/363624 |
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