Deep Synoptic Array Science: Two Fast Radio Burst Sources in Massive Galaxy Clusters

Deep Synoptic Array Science: Two Fast Radio Burst Sources in Massive Galaxy Clusters

The hot gas that constitutes the intracluster medium (ICM) has been studied at X-ray and millimeter/submillimeter wavelengths (Sunyaev–Zel’dovich effect) for decades. Fast radio bursts (FRBs) offer an additional method of directly measuring the ICM and gas surrounding clusters via observables such a...

Täydet tiedot

Bibliografiset tiedot
Päätekijät: Liam Connor, Vikram Ravi, Morgan Catha, Ge Chen, Jakob T. Faber, James W. Lamb, Gregg Hallinan, Charlie Harnach, Greg Hellbourg, Rick Hobbs, David Hodge, Mark Hodges, Casey Law, Paul Rasmussen, Jack Sayers, Kritti Sharma, Myles B. Sherman, Jun Shi, Dana Simard, Jean Somalwar, Reynier Squillace, Sander Weinreb, David P. Woody, Nitika Yadlapalli, The Deep Synoptic Array team
Aineistotyyppi: Artikkeli
Kieli:English
Julkaistu: IOP Publishing 2023-01-01
Sarja:The Astrophysical Journal Letters
Aiheet:
Intracluster medium
Radio bursts
Rich galaxy clusters
Linkit:https://doi.org/10.3847/2041-8213/acd3ea

Internet

https://doi.org/10.3847/2041-8213/acd3ea

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