Published May 21, 2025 | Version v1
Model Open

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

  • 1. ROR icon University of Portsmouth
  • 2. ROR icon Max Planck Institute for Astronomy
  • 3. ROR icon Kavli Institute for the Physics and Mathematics of the Universe
  • 4. ROR icon National Institute for Astrophysics

Description

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. 

 

Files

MaStar_plateifu.txt

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