Coma Cluster: CR Acceleration and Gamma-Ray Production

The Coma cluster is situated near to the North Pole and its galactic coordinates are: l ≃ 50° and b ≃87°. The distance to the cluster is about 138 Mpc. Observations in soft X-rays (see e.g. Briel, 1992) discovered there the thermal emission from the diffuse hot intracluster gas whose density and tem...

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Published in:Symposium - International Astronomical Union
Main Author: Dogiel, A.V.
Format: Article in Journal/Newspaper
Language:English
Published: Cambridge University Press (CUP) 1996
Subjects:
North Pole
Bazzano
Online Access:http://dx.doi.org/10.1017/s007418090008102x
https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S007418090008102X
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spelling crcambridgeupr:10.1017/s007418090008102x 2024-03-03T08:47:14+00:00 Coma Cluster: CR Acceleration and Gamma-Ray Production Dogiel, A.V. 1996 http://dx.doi.org/10.1017/s007418090008102x https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S007418090008102X en eng Cambridge University Press (CUP) https://www.cambridge.org/core/terms Symposium - International Astronomical Union volume 175, page 341-342 ISSN 0074-1809 journal-article 1996 crcambridgeupr https://doi.org/10.1017/s007418090008102x 2024-02-08T08:44:41Z The Coma cluster is situated near to the North Pole and its galactic coordinates are: l ≃ 50° and b ≃87°. The distance to the cluster is about 138 Mpc. Observations in soft X-rays (see e.g. Briel, 1992) discovered there the thermal emission from the diffuse hot intracluster gas whose density and temperature are: n≃ 3 · 10 –3 cm –3 and T≃ 10 8 K. Measurements of hard X-ray flux from Coma showed controversial detection in different experiments (see Bazzano et al. 1990 and Rephaeli et al. 1994). Article in Journal/Newspaper North Pole Cambridge University Press North Pole Bazzano ENVELOPE(-64.167,-64.167,-65.183,-65.183) Symposium - International Astronomical Union 175 341 342
institution Open Polar
collection Cambridge University Press
op_collection_id crcambridgeupr
language English
description The Coma cluster is situated near to the North Pole and its galactic coordinates are: l ≃ 50° and b ≃87°. The distance to the cluster is about 138 Mpc. Observations in soft X-rays (see e.g. Briel, 1992) discovered there the thermal emission from the diffuse hot intracluster gas whose density and temperature are: n≃ 3 · 10 –3 cm –3 and T≃ 10 8 K. Measurements of hard X-ray flux from Coma showed controversial detection in different experiments (see Bazzano et al. 1990 and Rephaeli et al. 1994).
format Article in Journal/Newspaper
author Dogiel, A.V.
spellingShingle Dogiel, A.V.
Coma Cluster: CR Acceleration and Gamma-Ray Production
author_facet Dogiel, A.V.
author_sort Dogiel, A.V.
title Coma Cluster: CR Acceleration and Gamma-Ray Production
title_short Coma Cluster: CR Acceleration and Gamma-Ray Production
title_full Coma Cluster: CR Acceleration and Gamma-Ray Production
title_fullStr Coma Cluster: CR Acceleration and Gamma-Ray Production
title_full_unstemmed Coma Cluster: CR Acceleration and Gamma-Ray Production
title_sort coma cluster: cr acceleration and gamma-ray production
publisher Cambridge University Press (CUP)
publishDate 1996
url http://dx.doi.org/10.1017/s007418090008102x
https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S007418090008102X
long_lat ENVELOPE(-64.167,-64.167,-65.183,-65.183)
geographic North Pole
Bazzano
geographic_facet North Pole
Bazzano
genre North Pole
genre_facet North Pole
op_source Symposium - International Astronomical Union
volume 175, page 341-342
ISSN 0074-1809
op_rights https://www.cambridge.org/core/terms
op_doi https://doi.org/10.1017/s007418090008102x
container_title Symposium - International Astronomical Union
container_volume 175
container_start_page 341
op_container_end_page 342
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