RXTE observations of GRB afterglows

被引：0

作者：

Marshall, FE

Swank, J

Valinia, A

Corbet, R

Takeshima, T

Barthelmy, S

Robinson, C

Kouveliotou, C

Connaughton, V

Kippen, M

Preece, R

Bradt, H

Levine, A

Remillard, R

Smith, D

Hurley, K

机构：

[1] NASA, Goddard Space Flight Ctr, High Energy Astrophys Lab, Greenbelt, MD 20771 USA

[2] Univ Space Res Assoc, Greenbelt, MD 20771 USA

[3] NASA, Goddard Space Flight Ctr, High Energy Astrophys Lab, Greenbelt, MD 20771 USA

[4] NASA, George C Marshall Space Flight Ctr, Huntsville, AL 35812 USA

[5] MIT, Ctr Space Res, Cambridge, MA 02138 USA

[6] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA

来源：

NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS | 1999年 / 69卷 / 1-3期

关键词：

D O I：

10.1016/S0920-5632(98)00314-4

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

Variable X-ray sources that appear to be the afterglows of the strong gamma-ray bursts GRB 970616 and GRB 970828 have been discovered with the RXTE PCA. First seen less than 4 hours after the burst, the flux from the sources decreased with time. Although near the sensitivity Limit of the PCA, the sources are the brightest afterglows yet seen in X-rays. Similar observations of two other bursts did not detect ang afterglows. These results are part of a continuing collaboration between RXTE, BATSE, and IPN scientists to rapidly detect X-ray afterglows of bright gamma-ray bursts.

引用

页码：640 / 645

页数：6

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