The Progenitor Systems of Classical Novae in M31

We present the first characterization of the statistical relationship between a large sample of novae in M31 and their progenitor stellar populations in the form of a delay time distribution. To this end, we leverage the spatially resolved stellar age distribution of the M31 disk derived from deep H...

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Bibliographic Details
Main Authors: C. S. Abelson, Carles Badenes, Laura Chomiuk, Benjamin F. Williams, Katelyn Breivik, L. Galbany, C. Jiménez-Palau
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
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Online Access:https://doi.org/10.3847/1538-4357/adc68c
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