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X-Ray Properties of LINERs and Low Luminosity Seyfert Galaxies Observed with ASCA

Published online by Cambridge University Press:  25 May 2016

Y. Terashima ,
H. Kunieda ,
P.J. Serlemitsos  and
A. Ptak
Y. Terashima
Affiliation:
Department of Physics, Nagoya University, Chikusa-ku, Nagoya, Japan
H. Kunieda
Affiliation:
Department of Physics, Nagoya University, Chikusa-ku, Nagoya, Japan
P.J. Serlemitsos
Affiliation:
Code 662, NASA/Goddard Space Flight Center, Greenbelt, MD 20771, USA
A. Ptak
Affiliation:
Code 662, NASA/Goddard Space Flight Center, Greenbelt, MD 20771, USA

Abstract

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We present ASCA spectra of low luminosity AGNs with X-ray luminosities of 1040-41 ergs s−1. Their X-ray continua are very similar to Seyfert galaxies. Although iron K emissin centered at 6.4 keV or 6.7 keV is detected from a few objects, iron K emission is weak on average. Possible reasons for variety of iron line properties are discussed.

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. 444 - 445
Copyright
Copyright © Kluwer 1998 

References

1. Ishisaki, et al. 1996, PASJ, 48, 237 Google Scholar
2. Makishima, et al. 1994, PASJ, 46, L77 Google Scholar
3. Ross, & Fabian, 1993, MNRAS, 261, 74 CrossRefGoogle Scholar
4. Serlemitsos, , Ptak, , & Yaqoob, 1996, in Physics of LINERs in view of Recent Observations, eds. Eracleous, et al.Google Scholar
5. Terashima, et al. 1997, in preparation Google Scholar
6. Życki, & Czerny, 1994, MNRAS, 266, 653 Google Scholar