Early-time γ -ray constraints on cosmic-ray acceleration in the core-collapse SN 2023ixf with the Fermi Large Area Telescope

被引：0

作者：

Martí-Devesa, G. ^{[1
,2
]}

Cheung, C.C. ^{[3
]}

Di Lalla, N. ^{[4
]}

Renaud, M. ^{[5
]}

Principe, G. ^{[2
,6
,7
]}

Omodei, N. ^{[4
]}

Acero, F. ^{[8
,9
]}

机构：

[1] Institut für Astro- und Teilchenphysik, Universität Innsbruck, Innsbruck,6020, Austria

[2] Dipartimento di Fisica, Universitá di Trieste, Trieste,34127, Italy

[3] Space Science Division, Naval Research Laboratory, Washington,DC,20375, United States

[4] W.W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics, SLAC National Accelerator Laboratory, Stanford University, Stanford,CA,94305, United States

[5] Laboratoire Univers et Particules de Montpellier (LUPM), Université de Montpellier, CNRS/IN2P3, CC72 Place Eugène Bataillon, Montpellier,34095 Cedex 5, France

[6] Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, Trieste,34127, Italy

[7] INAF - Istituto di Radioastronomia, Bologna,40129, Italy

[8] Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, Gif-sur-Yvette,91191, France

[9] FSLAC IRL 2009, CNRS/IAC, La Laguna, Tenerife, Spain

来源：

Astronomy and Astrophysics | 2024年 / 686卷

关键词：

Supernovae;

D O I：

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摘要：

Journal article (JA)

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