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X-ray and Gamma-ray Variability of NGC 1275

X-ray and Gamma-ray Variability of NGC 1275

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_doaj_primary_oai_doaj_org_article_f9f98cca62ef4a2391b04ff7fc6125f5

X-ray and Gamma-ray Variability of NGC 1275

About this item

Full title

X-ray and Gamma-ray Variability of NGC 1275

Publisher

Basel: MDPI AG

Journal title

Galaxies, 2020-09, Vol.8 (3), p.63

Language

English

Formats

Publication information

Publisher

Basel: MDPI AG

More information

Scope and Contents

Contents

Gamma-ray emission from the bright radio source 3C 84, associated with the Perseus cluster, is ascribed to the radio galaxy NGC 1275 residing at the centre of the cluster. Study of the correlated X-ray/gamma-ray emission from this active galaxy, and investigation of the possible disk-jet connection, are hampered because the X-ray emission, particul...

Alternative Titles

Full title

X-ray and Gamma-ray Variability of NGC 1275

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_doaj_primary_oai_doaj_org_article_f9f98cca62ef4a2391b04ff7fc6125f5

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_doaj_primary_oai_doaj_org_article_f9f98cca62ef4a2391b04ff7fc6125f5

Other Identifiers

ISSN

2075-4434

E-ISSN

2075-4434

DOI

10.3390/galaxies8030063

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