Abstract
A new bright gamma-ray source was detected in June 1995 near the Galactic plane (GRO J1838−04). Subsequent EGRET observations did not detect significant flux from this source. The gamma-ray error box of GRO J1838−04 does not contain any spectrally-flat radio-loud source. GRO J1838−04 provides strong evidence for the existence of a new class of variable gamma-ray sources.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
