Model data from "Stellar population modelling of neutron stars and black holes: spatially-resolved graveyards in MaNGA/SDSS-IV galaxies."

This repository contains models and modelled data from the publication "Stellar population modelling of neutron stars and black holes: spatially-resolved graveyards in MaNGA/SDSS-IV galaxies", MNRAS, 2025, These are: new stellar population models of remnant numbers and masses for evolving stellar populations as a function of metallicity and age, using a new Initial Mass - Final Mass relation from Limongi et al. 2018. The tables here refer to a Kroupa initial mass function. Models for other specific IMFs can be obtained upon request. the modelled data for spatially-resolved graveyards in MANGA galaxies. The new remnant models have been applied to spatially-resolved star formation histories of MANGA galaxies from Neumann et al. 2022 to obtain the distributions of stellar remnants in galaxies.

Related Organizations

Kavli Institute for the Physics and Mathematics of the Universe
Japan
University of Portsmouth
United Kingdom
Max Planck Society
Germany
National Institute for Astrophysics
Italy
Max Planck Institute for Astronomy
Germany

Impact byBIP!

	selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	0
	popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.	Average
	influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	Average
	impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.	Average

Found an issue? Give us feedback

0

Average