Pith. sign in

REVIEW

Gamma-rays and cosmic-rays from a pulsar in Cygnus OB2

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv astro-ph/0307216 v1 pith:4PLOZMMS submitted 2003-07-10 astro-ph

classification astro-ph
keywords pulsargamma-raysappearanceargueassociationcosmiccosmic-rayscreated
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

We argue that gamma-rays sources observed in the direction of the Cyg OB2 association in the GeV and TeV energy range are due to a pulsar which was created by a supernova a few tens of thousands years ago. The excess of cosmic rays at 10^18 eV can be also related to the appearance of this pulsar.

Discussion (0). Continue with ORCID to comment.

Pith tools