Supernova remnants as cosmic ray accelerators. SNR IC 443
We examine the hypothesis that some supernova remnants (SNRs) may be responsible for some unidentified y-ray sources detected by EGRET instrument aboard the Compton Gamma Ray Observatory. If this is the case, y-rays are produced via pion production and decay from direct inelastic collisions of a...
Gespeichert in:
Datum: | 1998 |
---|---|
Hauptverfasser: | , |
Format: | Artikel |
Sprache: | English |
Veröffentlicht: |
Інститут фізики конденсованих систем НАН України
1998
|
Schriftenreihe: | Condensed Matter Physics |
Online Zugang: | http://dspace.nbuv.gov.ua/handle/123456789/119813 |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
Zitieren: | Supernova remnants as cosmic ray accelerators. SNR IC 443 / B. Hnatyk, O. Petruk // Condensed Matter Physics. — 1998. — Т. 1, № 3(15). — С. 655-667. — Бібліогр.: 24 назв. — англ. |