Search for the Identification of 3EG J1835+5918: Evidence for a New Type of High-Energy Gamma-ray Source

TL;DR

This study investigates the unidentified gamma-ray source 3EG J1835+5918 through multiwavelength observations, revealing it lacks typical features of known gamma-ray emitters like blazars or pulsars, suggesting it may be a new type of high-energy source.

Contribution

The paper provides the first comprehensive multiwavelength analysis of 3EG J1835+5918, proposing it as a potentially new class of gamma-ray source due to its atypical properties.

Findings

No blazar-like or pulsar-like counterparts found.

Lacks typical radio and X-ray signatures of known gamma-ray sources.

May represent a new class of high-energy gamma-ray emitters.

Abstract

The EGRET source 3EG J1835+5918 is the brightest and most accurately positioned of the as-yet unidentified high-energy gamma-ray sources at high Galactic latitude (l,b=89,25). We present a multiwavelength study of the region around it, including X-ray, radio, and optical imaging surveys, as well as optical spectroscopic classification of most of the active objects in this area. The identified X-ray sources in or near the EGRET error ellipse are radio-quiet QSOs, a galaxy cluster, and coronal emitting stars. The radio sources inside the error ellipse are all fainter than 4 mJy at 1.4 GHz. In addition there are no flat-spectrum radio sources in the vicinity. Since no blazar-like or pulsar-like candidate has been found as a result of these searches, 3EG J1835+5918 must be lacking one or more of the physically essential attributes of these known classes of gamma-ray emitters. If it is an AGN it lacks the beamed radio emission of blazars by at least a factor of 100 relative to identified EGRET blazars. If it is an isolated neutron star, it lacks the steady thermal X-rays from a cooling surface and the magnetospheric non-thermal X-ray emission that is characteristic of all EGRET pulsars. If a pulsar, 3EG J1835+5918 must be either older or more distant than Geminga, and probably an even more efficient or beamed gamma-ray engine.