2025-02-22T17:15:35-05:00 DEBUG: VuFindSearch\Backend\Solr\Connector: Query fl=%2A&wt=json&json.nl=arrarr&q=id%3A%22ujp2-article-2019120%22&qt=morelikethis&rows=5
2025-02-22T17:15:35-05:00 DEBUG: VuFindSearch\Backend\Solr\Connector: => GET http://localhost:8983/solr/biblio/select?fl=%2A&wt=json&json.nl=arrarr&q=id%3A%22ujp2-article-2019120%22&qt=morelikethis&rows=5
2025-02-22T17:15:35-05:00 DEBUG: VuFindSearch\Backend\Solr\Connector: <= 200 OK
2025-02-22T17:15:35-05:00 DEBUG: Deserialized SOLR response
Комптонiзацiя космiчного мiкрохвильового випромiнювання холодним ультрарелятивiстським електрон-позитронним вiтром та природа ∼130 ГeВ лiнiй

Комптонiзацiя космiчного мiкрохвильового випромiнювання холодним ультрарелятивiстським електрон-позитронним вiтром та природа ∼130 ГeВ лiнiй

Previously, an astrophysical explanation of the narrow gamma-ray line-like feature(s) at ∼100 GeV from the Galactic Center region observed by Fermi/LAT [2] was proposed in [1]. The model of [1] is based on the inverse Compton scattering of external ultraviolet/X-ray radiation by a cold ultrarelativi...

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Bibliographic Details
Main Authors: Iakubovskyi, D., Yushchenko, S.
Format: Article
Language:English
Published: Publishing house "Academperiodika" 2019
Subjects:
gamma-ray line
Galactic Center
pulsar wind
inverse Compton effect
cosmic microwave background radiation
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Online Access:https://ujp.bitp.kiev.ua/index.php/ujp/article/view/2019120
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https://ujp.bitp.kiev.ua/index.php/ujp/article/view/2019120

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