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ASCA X-Ray Observation of the Lobe Dominant Radio Galaxy NGC 612

Published online by Cambridge University Press:  25 May 2016

M. Tashiro ,
H. Kaneda  and
K. Makishima
M. Tashiro
Affiliation:
Department of Physics, University of Tokyo Hongo 7-3-1, Tokyo, Japan 113-0033
H. Kaneda
Affiliation:
Department of Physics, University of Tokyo Hongo 7-3-1, Tokyo, Japan 113-0033
K. Makishima
Affiliation:
Department of Physics, University of Tokyo Hongo 7-3-1, Tokyo, Japan 113-0033

Extract

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The radio galaxy NGC 612 (z = 0.0290; Spinrad et al. 1985) exhibits bright (~ 11 Jy at 843 MHz) double lobes at a large scale of about 500 kpc x 130 kpc with a very faint core (Jones & McAdam 1992). We performed ASCA observations (AO-4; PI = Kaneda) of NGC 612 on July 12-14, 1996, in search for inverse-Compton (IC) X-rays from the radio lobes.

Type
Session 1: Plasma and Fresh Nucleosynthesis Phenomena
Information
Symposium - International Astronomical Union , Volume 188: The Hot Universe , 1998 , pp. 289 - 290
Copyright
Copyright © Kluwer 1998 

References

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