A closed-form formula for star formation histories in galactocentric radial shells is derived from empirical galaxy scaling relations and two star formation history models.
[17], see also [18–20], and the quenching prescription of Ref
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.GA 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Dark-matter-induced transients over cosmic time: The role of star formation history profiles
A closed-form formula for star formation histories in galactocentric radial shells is derived from empirical galaxy scaling relations and two star formation history models.