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The pulsar contribution to the diffuse galactic gamma-ray emission

Martin Pohl·Gottfried Kanbach·Stan D. Hunter·Brian B. Jones
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Abstract

There is active interest in the extent to which unresolved gamma-ray pulsars contribute to the galactic diffuse emission, and whether unresolved gamma-ray pulsars could be responsible for the excess of diffuse galactic emission above 1 GeV which has been observed by EGRET. The diffuse gamma-ray intensity due to unresolved pulsars is directly linked to the number of objects which should be observed in the EGRET data. We can therefore use our knowledge of the unidentified EGRET sources to constrain model parameters like the pulsar birth rate, their beaming angle, etc. This analysis is based only on the properties of the six pulsars which have been identified in the EGRET data, and is independent of choice of a pulsar emission model. We find that pulsars contribute very little to the diffuse emission at lower energies, whereas above 1 GeV they can account for 18% of the observed intensity in selected regions for a reasonable number of directly observable gamma-ray pulsars (14). The latitude distribution of the diffuse emission caused by unresolved pulsars is narrower than that of the observed diffuse emission. While the excess above 1 GeV gamma-ray energy is observed up to at least 6-8 degrees off the plane, the pulsar contribution would be small there. Thus pulsars do significantly contribute to the diffuse galactic gamma-ray emission above 1 GeV, but they can not be made responsible for all the discrepancy between observed intensity and model predictions in this energy range.

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Martin Pohl, Gottfried Kanbach, Stan D. Hunter, Brian B. Jones. 1997-11-17. The pulsar contribution to the diffuse galactic gamma-ray emission. https://arxiv.org/abs/astro-ph/9711183

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