Hostname: page-component-78c5997874-xbtfd Total loading time: 0 Render date: 2024-11-17T16:07:48.172Z Has data issue: false hasContentIssue false
  • English
  • Français

Stellar population synthesis of galaxies with chemical evolution model

Published online by Cambridge University Press:  10 June 2020

Shiyin Shen  and
Jun Yin
Shiyin Shen
Affiliation:
Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai, 200030, China Key Lab for Astrophysics, Shanghai, 200234, China email: [email protected]
Jun Yin
Affiliation:
Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai, 200030, China
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The derivation of accurate stellar populations of galaxies is a non-trivial task because of the well-known age-metallicity degeneracy. We aim to break this degeneracy by invoking a chemical evolution model (CEM) for isolated disk galaxy, where its metallicity enrichment history (MEH) is modelled to be tightly linked to its star formation history (SFH). Our CEM has been successfully tested on several local group dwarf galaxies whose SFHs and MEHs have been both independently measured from deep colour-magnitude diagrams of individual stars. By introducing the CEM into the stellar population fitting algorithm as a prior, we expect that the SFH of galaxies could be better constrained.

Keywords

galaxies: stellar contentgalaxies: evolutiongalaxies: abundances
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S341: Challenges in Panchromatic Modelling with Next Generation Facilities , November 2019 , pp. 147 - 151
Copyright
© International Astronomical Union 2020

References

Cid Fernandes, R., Mateus, A., Sodré, L., Stasińska, G., & Gomes, J. M. 2005, MNRAS, 358, 363CrossRefGoogle Scholar
Conroy, C. 2013, ARA&A, 51, 393CrossRefGoogle Scholar
Falcón-Barroso, J., Sánchez-Blázquez, P., Vazdekis, A., Ricciardelli, E., Cardiel, N., Cenarro, A.J., Gorgas, J., & Peletier, R. F. 2011, A&A, 532, A95Google Scholar
Gallart, C. 2007, Proceedings of the International Astronomical Union, 2Google Scholar
Kennicutt, R. C. 1998, ARA&A, 36, 189CrossRefGoogle Scholar
Ruiz-Lara, T., Pérez, I., Gallart, C., Alloin, D., Monelli, M., Koleva, M., Pompei, E., Beasley, M., et al. 2015, A&A, 583, A60Google Scholar
Ocvirk, P., Pichon, C., Lançon, A., & Thiébaut, E. 2006, MNRAS, 365, 74CrossRefGoogle Scholar