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- W2803024445 abstract "We have re-examined the properties of $gamma-$ray emitting globular clusters (GCs) with the data obtained by Fermi Large Area Telescope in the past nine years. With an updated sample of 19 $gamma-$ray GCs, we have performed a statistical analysis in the framework set by Hui et al. (2011) cite{hui}. We confirm that the correlation between the $gamma-$ray luminosities $L_{gamma}$ and the metalicity [Fe/H] is as significant as that between $L_{gamma}$ and the two-body encounter frequencies $Gamma_{c}$. Correlations between $L_{gamma}$ and the energy densities of the soft photon field $u_{rm optical}$/$u_{rm IR}$ at location of the GCs have also been confirmed. With a two-dimensional regression analysis, we have revised the fundamental planes of $gamma-$ray GCs which relate $L_{gamma}$, [Fe/H]/$Gamma_{c}$ and $u_{rm optical}$/$u_{rm IR}$. The updated relations based on can provide better prediction of the $gamma-$ray properties of GCs and support the scenario that the $gamma-$ray emission is originated from the inverse Compton scattering (ICS) between the pulsar wind and the ambient soft photon fields." @default.
- W2803024445 created "2018-05-17" @default.
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- W2803024445 date "2017-12-12" @default.
- W2803024445 modified "2023-09-25" @default.
- W2803024445 title "Reexamining the gamma-ray properties of globular clusters" @default.
- W2803024445 doi "https://doi.org/10.22323/1.312.0106" @default.
- W2803024445 hasPublicationYear "2017" @default.
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