Continuum and line emissions from the galactic ridge and clusters: Problems of interpretation and ways of solution

Vladimir A. Dogiel; Kuniaki Masai; Che Ming Ko; Ping Hung Kuo; Chorng Yuan Hwang; Wing Huen Ip

doi:10.1143/PTPS.169.131

Continuum and line emissions from the galactic ridge and clusters: Problems of interpretation and ways of solution

Vladimir A. Dogiel, Kuniaki Masai, Che Ming Ko, Ping Hung Kuo, Chorng Yuan Hwang, Wing Huen Ip

Graduate Institute of Astronomy

Research output: Contribution to journal › Article › peer-review

Abstract

The stochastic acceleration of subrelativistic electrons from background plasma is studied in order to find possible explanation of hard X-ray emission from the Galactic Ridge and galaxy clusters. From our analysis we show that the energy supply required to produce this emission is much less than it was obtained in the framework of previous models.

Original language	English
Pages (from-to)	131-135
Number of pages	5
Journal	Progress of Theoretical Physics Supplement
Issue number	169
DOIs	https://doi.org/10.1143/PTPS.169.131
State	Published - 2007

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title = "Continuum and line emissions from the galactic ridge and clusters: Problems of interpretation and ways of solution",

abstract = "The stochastic acceleration of subrelativistic electrons from background plasma is studied in order to find possible explanation of hard X-ray emission from the Galactic Ridge and galaxy clusters. From our analysis we show that the energy supply required to produce this emission is much less than it was obtained in the framework of previous models.",

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T2 - Problems of interpretation and ways of solution

AU - Dogiel, Vladimir A.

AU - Masai, Kuniaki

AU - Ko, Che Ming

AU - Kuo, Ping Hung

AU - Hwang, Chorng Yuan

AU - Ip, Wing Huen

PY - 2007

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AB - The stochastic acceleration of subrelativistic electrons from background plasma is studied in order to find possible explanation of hard X-ray emission from the Galactic Ridge and galaxy clusters. From our analysis we show that the energy supply required to produce this emission is much less than it was obtained in the framework of previous models.

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DO - 10.1143/PTPS.169.131

M3 - 期刊論文

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SN - 0375-9687

SP - 131

EP - 135

JO - Progress of Theoretical Physics Supplement

JF - Progress of Theoretical Physics Supplement

IS - 169

ER -

Continuum and line emissions from the galactic ridge and clusters: Problems of interpretation and ways of solution

Abstract

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