Repository logo
  • English
  • Italiano
Log In
Have you forgotten your password?
  1. Home
  2. PRODOTTI RICERCA INAF
  3. 1 CONTRIBUTI IN RIVISTE (Journal articles)
  4. 1.01 Articoli in rivista
  5. A dynamical view on stellar metallicity gradient diversity across the Hubble sequence with CALIFA
 

A dynamical view on stellar metallicity gradient diversity across the Hubble sequence with CALIFA

Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY  
Date Issued
2019
Author(s)
Zhuang, Yulong
•
Leaman, Ryan
•
van de Ven, Glenn
•
ZIBETTI, Stefano  
•
GALLAZZI, Anna Rita  
•
Zhu, Ling
•
Falcón-Barroso, Jesús
•
Lyubenova, Mariya
DOI
10.1093/mnras/sty2916
Abstract
We analyse radial stellar metallicity and kinematic profiles out to 1Re in 244 CALIFA galaxies ranging from morphological type E to Sd, to study the evolutionary mechanisms of stellar population gradients. We find that linear metallicity gradients exhibit a clear correlation with galaxy morphological type - with early-type galaxies showing the steepest gradients. We show that the metallicity gradients simply reflect the local mass-metallicity relation within a galaxy. This suggests that the radial stellar population distribution within a galaxy's effective radius is primarily a result of the in situ local star formation history. In this simple picture, the dynamically derived stellar surface mass density gradient directly predicts the metallicity gradient of a galaxy. We show that this correlation and its scatter can be reproduced entirely by using independent empirical galaxy structural and chemical scaling relations. Using Schwarzschild dynamical models, we also explore the link between a galaxy's local stellar populations and their orbital structures. We find that galaxies' angular momentum and metallicity gradients show no obvious causal link. This suggests that metallicity gradients in the inner disc are not strongly shaped by radial migration, which is confirmed by the lack of correlation between the metallicity gradients and observable probes of radial migration in the galaxies, such as bars and spiral arms. Finally, we find that galaxies with positive metallicity gradients become increasingly common towards low mass and late morphological types - consistent with stellar feedback more efficiently modifying the baryon cycle in the central regions of these galaxies.
Volume
483
Issue
2
Start page
1862
Uri
http://hdl.handle.net/20.500.12386/29356
Url
https://academic.oup.com/mnras/article/483/2/1862/5181346
Issn Identifier
0035-8711
Ads BibCode
2019MNRAS.483.1862Z
Rights
open.access
File(s)
Loading...
Thumbnail Image
Name

sty2916.pdf

Description
pdf editoriale
Size

3.59 MB

Format

Adobe PDF

Checksum (MD5)

f9eb515dd1970fc537c5ba2072c9c910

Loading...
Thumbnail Image
Name

1810.12223.pdf

Description
preprint
Size

6.99 MB

Format

Adobe PDF

Checksum (MD5)

3a58c9470c82d11e9d5eb93e2296d019

Explore By
  • Communities and Collection
  • Research Outputs
  • Researchers
  • Organizations
  • Projects
Information and guides for authors
  • https://openaccess-info.inaf.it: all about open access in INAF
  • How to enter a product: guides to OA@INAF
  • The INAF Policy on Open Access
  • Downloadable documents and templates

Built with DSpace-CRIS software - Extension maintained and optimized by 4Science

  • Privacy policy
  • End User Agreement
  • Send Feedback