η Carinae with Fermi-LAT: two full orbits and the third periastron

G Martí-Devesa, O Reimer - Astronomy & Astrophysics, 2021 - aanda.org
Context. Colliding-wind binaries are massive stellar systems featuring strong, interacting
winds. These binaries may be actual particle accelerators, making them variable γ-ray …
被引用次数：15 相关文章

Eta Carinae with Fermi-LAT: Two full orbits and the third periastron

G Martí-Devesa, O Reimer - arXiv preprint arXiv:2109.05950, 2021 - arxiv.org
Context. Colliding-wind binaries are massive stellar systems featuring strong, interacting
winds. These binaries may be actual particle accelerators, making them variable gamma-ray …

η Carinae with Fermi-LAT: two full orbits and the third periastron

G Martí-Devesa, O Reimer - Astronomy and Astrophysics, 2021 - ui.adsabs.harvard.edu
Context. Colliding-wind binaries are massive stellar systems featuring strong, interacting
winds. These binaries may be actual particle accelerators, making them variable γ-ray …
[PDF] archive.org

[PDF][PDF] η Carinae with Fermi-LAT: two full orbits and the third periastron

G Martí-Devesa, O Reimer - A&A, 2021 - scholar.archive.org
Context. Colliding-wind binaries are massive stellar systems featuring strong, interacting
winds. These binaries may be actual particle accelerators, making them variable γ-ray …

η Carinae with Fermi-LAT: two full orbits and the third periastron

G Martí-Devesa, O Reimer - Astron. Astrophys., 2021 - inspirehep.net
Context. Colliding-wind binaries are massive stellar systems featuring strong, interacting
winds. These binaries may be actual particle accelerators, making them variable γ-ray …

η Carinae with Fermi-LAT: two full orbits and the third periastron

G Martí-Devesa, O Reimer - Astronomy and Astrophysics, 2021 - ui.adsabs.harvard.edu
Context. Colliding-wind binaries are massive stellar systems featuring strong, interacting
winds. These binaries may be actual particle accelerators, making them variable γ-ray …