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Radial resolved galaxy disks models based on semi-analytic models of galaxy formation

Published online by Cambridge University Press:  10 June 2020

Jian Fu
Jian Fu*
Affiliation:
Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, CAS, 80 Nandan Road., Shanghai, 200030, China email: [email protected]
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Abstract

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We show our work on the L-Galaxies semi-analytic models of galaxy formation, which includes the radial resolved distribution of star, gas, SFR and metallicity on each galaxy disk. The newest version of the codes include the H22-to-HI gas transition prescriptions and the chemical enrichment of various elements. Our revised model can give results on cold gas components, radial metallicity gradients and scaling relations, which can fit the recent observations.

Keywords

galaxies: formationgalaxies: ISMISM: atomsgalaxies: 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. 273 - 274
Copyright
© International Astronomical Union 2020

Footnotes

†

Supported by Natural Science Foundation of China (No. U1531123) and the Youth innovation Promotion Association, Chinese Academy of Sciences.

References

Fu, J., Kauffmann, G., Huang, M.-L., et al. 2013, MNRAS, 434, 153110.1093/mnras/stt1117CrossRefGoogle Scholar
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Yates, R. M. & Kauffmann, G. 2014, MNRAS, 439, 381710.1093/mnras/stu233CrossRefGoogle Scholar
Henriques, B. M., Yates, R. M., Fu, J., et al. 2020, MNRAS, 491, 5795HCrossRefGoogle Scholar