On the evolution of simulated galaxies: the mass dependence in metallicity gradients

E-ISSN： 1743-9221|11|S321|302-302

ISSN： 1743-9213

Source： Proceedings of the International Astronomical Union, Vol.11, Iss.S321, 2017-03, pp. : 302-302

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Abstract

Related content

What shapes stellar metallicity gradients of massive galaxies at large radii?

Proceedings of the International Astronomical Union, Vol. 11, Iss. S321, 2017-03 ,pp. : 93-95

Cambridge University Press

Access to resources Recommend Favorite

The mass-metallicity relation of absorption selected high-redshift galaxies

Proceedings of the International Astronomical Union, Vol. 11, Iss. S321, 2017-03 ,pp. : 357-359

Cambridge University Press

Access to resources Recommend Favorite

Real Simulated IFU Observations of Low-Mass Early-Type Galaxies: Environmental Influence Probed for Cluster Galaxies

Proceedings of the International Astronomical Union, Vol. 11, Iss. S321, 2017-03 ,pp. : 289-289

Cambridge University Press

Access to resources Recommend Favorite

Dust and Metallicity across local Galaxies

Proceedings of the International Astronomical Union, Vol. 11, Iss. A29B, 2016-10 ,pp. : 176-177

Cambridge University Press

Access to resources Recommend Favorite

Giant disk galaxies : Where environment trumps mass in galaxy evolution

Proceedings of the International Astronomical Union, Vol. 11, Iss. A29B, 2016-10 ,pp. : 738-738

Cambridge University Press

Access to resources Recommend Favorite