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Pegasus W: An Ultrafaint Dwarf Galaxy Outside the Halo of M31 Not Quenched by Reionization

We report the discovery of an ultrafaint dwarf (UFD) galaxy, Pegasus W, located on the far side of the Milky Way–M31 system and outside the virial radius of M31. The distance to the galaxy is ${915}_{-91}^{+60}$ kpc, measured using the luminosity of horizontal branch stars identified in Hubble Space...

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Bibliografische gegevens
Hoofdauteurs: Kristen B. W. McQuinn, Yao-Yuan Mao, Matthew R. Buckley, David Shih, Roger E. Cohen, Andrew E. Dolphin
Formaat: Artigo
Taal:Inglês
Gepubliceerd in: IOP Publishing 2023-01-01
Reeks:The Astrophysical Journal
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Online toegang:https://doi.org/10.3847/1538-4357/acaec9
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