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The Initial-to-final Mass Relation of White Dwarfs in Intermediate-separation Binaries

We examine the applicability of the initial-to-final mass relation (IFMR) for white dwarfs (WDs) in intermediate-separation binary systems (∼1 au), using astrometric binaries identified in open clusters from Gaia DR3. A careful analysis of the astrometric orbits and spectral energy distributions iso...

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Bibliográfalaš dieđut
Váldodahkkit: Oren Ironi, Sagi Ben-Ami, Na’ama Hallakoun, Sahar Shahaf
Materiálatiipa: Artigo
Giella:Inglês
Almmustuhtton: IOP Publishing 2025-01-01
Ráidu:The Astrophysical Journal
Fáttát:
Liŋkkat:https://doi.org/10.3847/1538-4357/adb5f2
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