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ASCA Observations of the Superluminal Jet Source GRS1915+105

Published online by Cambridge University Press:  25 May 2016

Ken Ebisawa ,
T. Takeshima ,
N. E. White ,
T. Kotani ,
T. Dotani ,
Y. Ueda ,
B. A. Harmon ,
C. R. Robinson ,
S. N. Zhang  and
W. S. Paciesas
...Show all authors
Ken Ebisawa
Affiliation:
Laboratory for High Energy Astrophysics, NASA/GSFC Greenbelt, MD, 20771, USA
T. Takeshima
Affiliation:
Laboratory for High Energy Astrophysics, NASA/GSFC Greenbelt, MD, 20771, USA
N. E. White
Affiliation:
Laboratory for High Energy Astrophysics, NASA/GSFC Greenbelt, MD, 20771, USA
T. Kotani
Affiliation:
The Institute of Physical and Chemical Research (RIKEN) 2-1 Hirosawa, Wako, Saitama, 351-01, Japan
T. Dotani
Affiliation:
Institute of Space and Astronautical Science Yoshinodai, Sagamihara, Kanagawa, 229, Japan
Y. Ueda
Affiliation:
Institute of Space and Astronautical Science Yoshinodai, Sagamihara, Kanagawa, 229, Japan
B. A. Harmon
Affiliation:
NASA/MSFC Huntsville, AL 35806, USA
C. R. Robinson
Affiliation:
NASA/MSFC Huntsville, AL 35806, USA
S. N. Zhang
Affiliation:
NASA/MSFC Huntsville, AL 35806, USA
W. S. Paciesas
Affiliation:
Department of Physics, University of Alabama in Huntsville Huntsville, AL 35899, USA
M. Tavani
Affiliation:
Columbia Astrophysics Laboratory, Columbia University New York, NY 10027, USA
R. Foster
Affiliation:
Naval Research Laboratory Washington C. C. 20375, USA

Extract

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GRS1915+105 is an extraordinary X-ray transient which exhibits superluminal radio jets. In this paper, ASCA observations of the GRS1915+105 conducted from 1994 to 1997 are reported. Observations are carried out on the following dates each for ~ 20 ksec exposure; Sep 27 1994, April 20 1995, Oct 23 1996 and Apr 25 1997.

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. 392 - 393
Copyright
Copyright © Kluwer 1998