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arXiv Astrophysics

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5h ago

From observing strategies to velocity dispersion bias: forward modeling unresolved binaries in ultra-faint dwarf galaxiestranslating…

arXiv:2609.19407v1 Announce Type: new 
Abstract: Ultra-faint dwarf galaxies (UFDs) in the Milky Way are ideal probes of low-mass galaxy formation and dark matter because they are highly dark-matter dominated. In the lowest-mass systems, however, unresolved binary orbital motion…

Factuality

70/100

Political Bias

Lean Right

Ownership

arXiv Media House

Country

Unknown

Keywords#dwarf galaxies#ultra-faint dwarf#unresolved#science

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From observing strategies to velocity dispersion bias: forward modeling unresolved binaries in ultra-faint dwarf galaxies | Pulse Aggregator