Gamma-ray emission from high Galactic latitude globular clusters

被引:15
作者
Lloyd, Sheridan J. [1 ]
Chadwick, Paula M. [1 ]
Brown, Anthony M. [1 ]
机构
[1] Univ Durham, Ctr Adv Instrumentat, Dept Phys, South Rd, Durham DH1 3LE, England
基金
英国科学技术设施理事会;
关键词
astroparticle physics; pulsars: general; globular clusters: general; gamma-rays: general; LARGE-AREA TELESCOPE; MILLISECOND PULSARS; 47; TUCANAE; MILKY-WAY; NGC; 6752; FERMI; COUNTERPARTS; POPULATION; ORIGIN; MASSES;
D O I
10.1093/mnras/sty2150
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We analyse 8 yr of PASS 8 Fermi-LAT data, in the 60 MeV-300 GeV energy range, from 30 high Galactic latitude globular clusters. Six of these globular clusters are detected with a TS > 25, with NGC 6254 being detected as gamma-ray bright for the first time. The most significant detection is of the well-known globular cluster 47 Tuc, and we produce a refined spectral fit for this object with a log parabola model. NGC 6093, NGC 6752, and NGC 6254 are fitted with hard, flat power-law models. NGC 7078 is best fitted with a soft power law, and NGC 6218 is best fitted with a hard, broken power law. This variety of spectral models suggests that there is a variety of gamma-ray source types within globular clusters, in addition to the traditional millisecond pulsar interpretation. We identify a correspondence between diffuse X-ray emission in globular cluster cores and gamma-ray emission. This connection suggests that gamma-ray emission in globular clusters could also arise from unresolved X-ray sources or a relativistic electron population, perhaps generated by the millisecond pulsars. X-ray observations of further gamma-ray bright globular clusters would allow a functional relationship to be determined between diffuse X-ray and gamma-ray emission.
引用
收藏
页码:4782 / 4796
页数:15
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