Bibcode
Cano-Díaz, M.; Sánchez, S. F.; Zibetti, S.; Ascaribar, Y.; Bland-Hawthorn, J.; Ziegler, B.; González-Delgado, R. M.; Walcher, C. J.; García-Benito, R.; Mast, D.; Mendoza-Pérez, M. A.; Falcón-Barroso, J.; Galbany, L.; Husemann, B.; Kehring, C.; Marino, R. A.; Sánchez-Blázquez, P.; López-Cobá, C.; López-Sánchez, A. R.; Vilchez, J. M.
Bibliographical reference
Proceeding of the conference The Interplay between Local and Global Processes in Galaxies, Cozumel, Mexico, 2016-4, Eds. S. F. Sanchez, C. Morisset and G. Delgado-Inglada
Advertised on:
6
2016
Citations
0
Refereed citations
0
Description
The relation known as Star Formation Main Sequence (SFMS) of galaxies is
defined in terms of stellar mass and star formation rate. This
approximately linear relation has been proven to be tight and holds for
several star formation indicators at local and at high redshifts. In
this talk I will show recent results about our first attempts to study
the Spatially Resolved SFMS, using integral field spectroscopic data,
coming primarily from the CALIFA survey. I will present as a main result
that a local SFMS is found with a slope and zero point of 0.72 +/ 0.04,
and -7.95 +/ 0.29 respectively. I will also discuss the influence of
characteristics such as environment and morphology in the relation.
Finally I will present some extensions of these results for data com in
from the MaNGA survey.