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The evolution of the oxygen radial gradients in spiral galaxies

Published online by Cambridge University Press:  03 March 2020

M. Mollá ,
O. Cavichia ,
B. Gibson ,
P. Tissera ,
P. Sánchez-Blázquez ,
A. I. Díaz ,
Y. Ascasibar ,
C. G. Few ,
S. F. Sánchez  and
W. J. Maciel
M. Mollá
Affiliation:
Depto. de Investigación Básica, CIEMAT, Avda. Complutense 40. E-28040 Madrid. (Spain) email: [email protected]
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Abstract

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We analyse the evolution with redshift of the radial gradient of oxygen abundances in spiral disks resulting from our MULCHEM chemical evolution models, computed for galaxies of different sizes or masses, studying the relationships between the gradients and galaxy characteristics as the stellar mass, the size, the gas fraction or the star formation rate for z < 4.

Keywords

Galaxies: SpiralsGalaxies: AbundancesGalaxies: Formation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium A30: Astronomy in Focus XXX , August 2018 , pp. 265
Copyright
© International Astronomical Union 2020

References

Mollá, M., Cavichia, O., Gavilán, M., Gibson, B. K. 2015, MNRAS, 451, 3693 CrossRefGoogle Scholar
Mollá, M., Daz, Á. I., Gibson, B. K., Cavichia, O., et al. 2016, MNRAS, 462, 1329 CrossRefGoogle Scholar
Mollá, M., Daz, Á. I., Ascasibar, Y., Gibson, B. K. 2017, MNRAS, 468, 305 CrossRefGoogle Scholar
Mollá, M., Daz, A. I., Cavichia, O., Gibson, B. K., et al. 2019, MNRAS, 482, 307 Google Scholar