FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3099088954> ?p ?o ?g. }

• W3099088954 endingPage "A82" @default.
• W3099088954 startingPage "A82" @default.
• W3099088954 abstract "<i>Context. <i/>The Gamma-ray emission from galaxy clusters hosting active galaxies is a complex combination of diffuse and point-like emission features with different spectral and spatial properties.<i>Aims. <i/>We discuss in details the case of the Perseus cluster containing the radio-galaxy NGC 1275 that has been recently detected as a bright gamma-ray source by the <i>Fermi<i/>-LAT experiment, in order to disentangle the sources of emission.<i>Methods. <i/>We provide a detailed study of the gamma-ray emission coming from the core of Perseus by modeling the central AGN emission with a multiple plasma blob model, and the emission from the extended cluster atmosphere with both a warming ray (WR) model and dark matter (DM) neutralino annihilation models. We set constraints on both the central galaxy and cluster SED models by using both archival multi-frequency data and the recent very high energy observations obtained by Fermi and MAGIC.<i>Results. <i/>We find that: i) in all the viable models for the cluster gamma-ray emission, the emission detected recently by Fermi from the center of the Perseus cluster is dominated by the active galaxy NGC 1275, that is found in a high-emission state; ii) the diffuse gamma-ray emission of the cluster, in the WR model and in the DM models with the highest allowed normalization, could be detected by Fermi if the central emission from NGC 1275 is in a low-emission state; iii) Fermi can have the possibility to resolve and detect the diffuse gamma-ray flux (predicted by the WR model) coming from the outer corona of the Perseus cluster atmosphere at distances <i>r<i/> 800 kpc. These results are consistent with the evidence that in the other frequency bands, the diffuse cluster emission dominates on the central galaxy one at low radio frequencies with <i>ν<i/> 1 GHz and at X-ray energies of order of <i>E<i/>~ keV.<i>Conclusions. <i/>Our results show that a simultaneous study of the various emission mechanisms that produce diffuse gamma-rays from galaxy clusters and the study of the emission mechanisms that produce gamma-rays from active galaxies residing in the cluster atmospheres is absolutely crucial first to disentangle the spectral and spatial characteristics of the gamma-ray emission and secondly to assess the optimal observational strategy in the attempt to reveal the still elusive diffuse gamma-ray emission widely predicted for the atmospheres of large-scale structures." @default.
• W3099088954 created "2020-11-23" @default.
• W3099088954 creator A5040747406 @default.
• W3099088954 creator A5047793211 @default.
• W3099088954 creator A5061729976 @default.
• W3099088954 date "2010-09-01" @default.
• W3099088954 modified "2023-10-18" @default.
• W3099088954 title "Disentangling the gamma-ray emission of NGC 1275 and that of the Perseus cluster" @default.
• W3099088954 cites W1967137800 @default.
• W3099088954 cites W1974849479 @default.
• W3099088954 cites W1984302612 @default.
• W3099088954 cites W1989762565 @default.
• W3099088954 cites W1990612862 @default.
• W3099088954 cites W1990940601 @default.
• W3099088954 cites W1994236395 @default.
• W3099088954 cites W1997587116 @default.
• W3099088954 cites W2001201254 @default.
• W3099088954 cites W2005789793 @default.
• W3099088954 cites W2009112801 @default.
• W3099088954 cites W2013433499 @default.
• W3099088954 cites W2017421813 @default.
• W3099088954 cites W2020716432 @default.
• W3099088954 cites W2023897244 @default.
• W3099088954 cites W2025487040 @default.
• W3099088954 cites W2028766997 @default.
• W3099088954 cites W2037741652 @default.
• W3099088954 cites W2040481874 @default.
• W3099088954 cites W2054266069 @default.
• W3099088954 cites W2054996930 @default.
• W3099088954 cites W2070078220 @default.
• W3099088954 cites W2074716047 @default.
• W3099088954 cites W2082072943 @default.
• W3099088954 cites W2089422028 @default.
• W3099088954 cites W2093932888 @default.
• W3099088954 cites W2099782510 @default.
• W3099088954 cites W2102608719 @default.
• W3099088954 cites W2117221941 @default.
• W3099088954 cites W2119708244 @default.
• W3099088954 cites W2136517687 @default.
• W3099088954 cites W2139710440 @default.
• W3099088954 cites W2144696109 @default.
• W3099088954 cites W2145269049 @default.
• W3099088954 cites W2148991125 @default.
• W3099088954 cites W2153481812 @default.
• W3099088954 cites W2154811628 @default.
• W3099088954 cites W2156048499 @default.
• W3099088954 cites W2159841242 @default.
• W3099088954 cites W2162132003 @default.
• W3099088954 cites W2164930427 @default.
• W3099088954 cites W2399949365 @default.
• W3099088954 cites W3098333105 @default.
• W3099088954 cites W3098637698 @default.
• W3099088954 cites W3098667313 @default.
• W3099088954 cites W3099405871 @default.
• W3099088954 cites W3100358084 @default.
• W3099088954 cites W3100959131 @default.
• W3099088954 cites W3101858791 @default.
• W3099088954 cites W3102269040 @default.
• W3099088954 cites W3102970791 @default.
• W3099088954 cites W3103254780 @default.
• W3099088954 cites W3103470394 @default.
• W3099088954 cites W3103550344 @default.
• W3099088954 cites W3103721591 @default.
• W3099088954 cites W3104150504 @default.
• W3099088954 cites W3104652416 @default.
• W3099088954 cites W3105180953 @default.
• W3099088954 cites W3105654390 @default.
• W3099088954 doi "https://doi.org/10.1051/0004-6361/201014393" @default.
• W3099088954 hasPublicationYear "2010" @default.
• W3099088954 type Work @default.
• W3099088954 sameAs 3099088954 @default.
• W3099088954 citedByCount "14" @default.
• W3099088954 countsByYear W30990889542012 @default.
• W3099088954 countsByYear W30990889542013 @default.
• W3099088954 countsByYear W30990889542014 @default.
• W3099088954 countsByYear W30990889542015 @default.
• W3099088954 countsByYear W30990889542016 @default.
• W3099088954 countsByYear W30990889542017 @default.
• W3099088954 countsByYear W30990889542019 @default.
• W3099088954 crossrefType "journal-article" @default.
• W3099088954 hasAuthorship W3099088954A5040747406 @default.
• W3099088954 hasAuthorship W3099088954A5047793211 @default.
• W3099088954 hasAuthorship W3099088954A5061729976 @default.
• W3099088954 hasBestOaLocation W30990889541 @default.
• W3099088954 hasConcept C121332964 @default.
• W3099088954 hasConcept C1276947 @default.
• W3099088954 hasConcept C156055797 @default.
• W3099088954 hasConcept C186769553 @default.
• W3099088954 hasConcept C20249676 @default.
• W3099088954 hasConcept C44870925 @default.
• W3099088954 hasConcept C98444146 @default.
• W3099088954 hasConceptScore W3099088954C121332964 @default.
• W3099088954 hasConceptScore W3099088954C1276947 @default.
• W3099088954 hasConceptScore W3099088954C156055797 @default.
• W3099088954 hasConceptScore W3099088954C186769553 @default.
• W3099088954 hasConceptScore W3099088954C20249676 @default.
• W3099088954 hasConceptScore W3099088954C44870925 @default.
• W3099088954 hasConceptScore W3099088954C98444146 @default.

• next