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10.7. Absorption columns with bright X-ray sources near the galactic center: — mass estimation in the Galactic center region

Published online by Cambridge University Press:  25 May 2016

Masaaki Sakano
Affiliation:
Department of Physics, Kyoto University, Sakyo, Kyoto, Japan
Mamiko Nishiuchi
Affiliation:
Department of Physics, Kyoto University, Sakyo, Kyoto, Japan
Yoshitomo Maeda
Affiliation:
Department of Physics, Kyoto University, Sakyo, Kyoto, Japan
Katsuji Koyama
Affiliation:
Department of Physics, Kyoto University, Sakyo, Kyoto, Japan
Jun Yokogawa
Affiliation:
Department of Physics, Kyoto University, Sakyo, Kyoto, Japan

Abstract

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We report the column density distribution to the Galactic Center region using the X-ray binary observations with the X-ray satellite ASCA, and demonstrate a new method of the total mass determination near the Galactic Center. The column densities are given by a simple form as a function of the angular distance from the Galactic Plane. Assuming a disklike mass distribution of 500 pc radius, we estimate the total mass to be ~ 6 × 107M.

Type
Part III. Black Holes and Central Activity
Copyright
Copyright © Kluwer 1998 

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