Gamma-ray spectral properties of the Galactic globular clusters: constraint on the numbers of millisecond pulsars
Wei Wu (1), Zhongxiang Wang (1,2), Yi Xing (2), Pengfei Zhang (1) (1., Yunnan University, 2. Shanghai Astronomical Observatory)

TL;DR
This study analyzes gamma-ray spectra of 30 globular clusters using Fermi data, modeling MSP contributions to understand their numbers and spectral properties, revealing that encounter rate alone doesn't determine MSP populations.
Contribution
The paper introduces a spectral model for gamma-ray emission from MSPs in globular clusters and estimates MSP numbers, comparing them with radio observations and highlighting factors influencing MSP populations.
Findings
27 GCs' gamma-ray spectra explained by MSPs
Estimated MSP numbers align with radio observations
Encounter rate is not the sole factor for MSP abundance
Abstract
We study the gamma-ray spectra of 30 globular clusters (GCs) thus far detected with the Fermi Gamma-ray Space Telescope. Presuming that gamma-ray emission of a GC comes from millisecond pulsars (MSPs) contained in, a model that generates spectra for the GCs is built based on the gamma-ray properties of the detected MSP sample. We fit the GCs' spectra with the model, and for 27 of them, their emission can be explained with arising from MSPs. The spectra of the other three, NGC 7078, 2MS-GC01, and Terzan 1, can not be fit with our model, indicating that MSPs' emission should not be the dominant one in the first two and the third one has a unique hard spectrum. We also investigate six nearby GCs that have relatively high encounter rates as the comparison cases. The candidate spectrum of NGC 6656 can be fit with that of one MSP, supporting its possible association with the gamma-ray source…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Pulsars and Gravitational Waves Research · Gamma-ray bursts and supernovae
