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Quick Observations of the Fading X-Rays from Gamma-Ray Bursts with ASCA

Published online by Cambridge University Press:  25 May 2016

T. Murakami ,
Y. Ueda ,
R. Fujimoto ,
M. Ishida ,
R. Shibata ,
S. Uno ,
F. Nagase ,
A. Yoshida ,
N. Kawai  and
F. Tokani
...Show all authors
T. Murakami
Affiliation:
Institute of Space and Astronautical Science 3-1-1, Yoshinodai, Sagamihara, Kanagawa 229, Japan
Y. Ueda
Affiliation:
Institute of Space and Astronautical Science 3-1-1, Yoshinodai, Sagamihara, Kanagawa 229, Japan
R. Fujimoto
Affiliation:
Institute of Space and Astronautical Science 3-1-1, Yoshinodai, Sagamihara, Kanagawa 229, Japan
M. Ishida
Affiliation:
Institute of Space and Astronautical Science 3-1-1, Yoshinodai, Sagamihara, Kanagawa 229, Japan
R. Shibata
Affiliation:
Institute of Space and Astronautical Science 3-1-1, Yoshinodai, Sagamihara, Kanagawa 229, Japan
S. Uno
Affiliation:
Institute of Space and Astronautical Science 3-1-1, Yoshinodai, Sagamihara, Kanagawa 229, Japan
F. Nagase
Affiliation:
Institute of Space and Astronautical Science 3-1-1, Yoshinodai, Sagamihara, Kanagawa 229, Japan
A. Yoshida
Affiliation:
Institute of Physical and Chemical Research 2-1, Hirosawa, Wako, Saitama 351, Japan
N. Kawai
Affiliation:
Institute of Physical and Chemical Research 2-1, Hirosawa, Wako, Saitama 351, Japan
F. Tokani
Affiliation:
Institute of Physical and Chemical Research 2-1, Hirosawa, Wako, Saitama 351, Japan
C. Otani
Affiliation:
Institute of Physical and Chemical Research 2-1, Hirosawa, Wako, Saitama 351, Japan
F.E. Marshall
Affiliation:
The Large International Collaborations
R.H.D. Corbet
Affiliation:
The Large International Collaborations
J.H. Swank
Affiliation:
The Large International Collaborations
T. Takeshima
Affiliation:
The Large International Collaborations
D.A. Smith
Affiliation:
The Large International Collaborations
A. Levine
Affiliation:
The Large International Collaborations
R.A. Remillard
Affiliation:
The Large International Collaborations
R. Vanderspek
Affiliation:
The Large International Collaborations
C.R. Robinson
Affiliation:
The Large International Collaborations
C. Kouveliotou
Affiliation:
The Large International Collaborations
C. Meegan
Affiliation:
The Large International Collaborations
V. Connaughton
Affiliation:
The Large International Collaborations
R.M. Kippen
Affiliation:
The Large International Collaborations
K. Hurley
Affiliation:
The Large International Collaborations
S.D. Barthelmy
Affiliation:
The Large International Collaborations
L. Piro
Affiliation:
The Large International Collaborations
E. Costa
Affiliation:
The Large International Collaborations
J. Heise
Affiliation:
The Large International Collaborations
F. Fiore
Affiliation:
The Large International Collaborations
J.V. Paradijs
Affiliation:
The Large International Collaborations
Y. Tanaka
Affiliation:
The Large International Collaborations
J. Greiner
Affiliation:
The Large International Collaborations
Isas Team
Affiliation:
Institute of Space and Astronautical Science 3-1-1, Yoshinodai, Sagamihara, Kanagawa 229, Japan
Riken Team
Affiliation:
Institute of Physical and Chemical Research 2-1, Hirosawa, Wako, Saitama 351, Japan
Rxte Team
Affiliation:
The Large International Collaborations
Batse Team
Affiliation:
The Large International Collaborations
UCB
Affiliation:
The Large International Collaborations
GCN
Affiliation:
The Large International Collaborations
SAX Team
Affiliation:
The Large International Collaborations
UOA
Affiliation:
The Large International Collaborations
AIP
Affiliation:
The Large International Collaborations

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Since the discovery of fading X-rays from Gamma-Ray Bursts (GRBs) with BeppoSAX (Piro et al. 1997, Costa et al. 1997), world-wide follow-up observations in optical band have achieved the fruitful results. The case of GRB 970228, there was an optical transient, coincides with the BeppoSAX position and faded (Paradijs et al. 1997, Sahu et al. 1997). These optical observations also confirmed the extended component, which was associated with the optical transient. The new transient are fading with a power-law function in time and the later observation of HST confirmed the extended emission is stable (Fruchter et al. 1997). This extended object seems to be a distant galaxy and strongly suggests to be the host.

Type
Session 3: Diagnostics of High Gravity Objects with X- and Gamma Rays
Information
Symposium - International Astronomical Union , Volume 188: The Hot Universe , 1998 , pp. 171 - 174
Copyright
Copyright © Kluwer 1998 

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