dc.citation.conferencePlace |
SP |
- |
dc.citation.conferencePlace |
Toledo, Spain |
- |
dc.citation.endPage |
171 |
- |
dc.citation.startPage |
163 |
- |
dc.citation.title |
IAU Symposium- Formation and Evolution of Galaxy Outskirts |
- |
dc.contributor.author |
Carollo, C. M. |
- |
dc.contributor.author |
Erroz-Ferrer, S. |
- |
dc.contributor.author |
den Brok, M. |
- |
dc.contributor.author |
Fagioli, M. |
- |
dc.contributor.author |
Onodera, M. |
- |
dc.contributor.author |
Tacchella, Sandro |
- |
dc.date.accessioned |
2023-12-19T21:08:23Z |
- |
dc.date.available |
2023-12-19T21:08:23Z |
- |
dc.date.created |
2021-07-27 |
- |
dc.date.issued |
2016-03 |
- |
dc.description.abstract |
We present the MUSE Atlas of Disks (MAD), a GTO program with the MUSE spectrograph on the ESO/VLT that is dedicated to the study of the optical spectroscopic properties of z = 0 disk galaxies on the star-forming ‘Main Sequence’ at < 100 pc physical resolution. MUSE pointings on the MAD galaxies extend out to ~ 2 disk scale lengths, enabling to investigate the bulge and inner disk properties of galaxies with different outer disks. Here we specifically compare, at constant stellar-mass, the stellar population properties of the inner components in disks with down-bending (Type II) and up-bending (Type III) outer profiles. We highlight similarities in the inner stellar properties of such different hosts, which point at a universal inside-out growth of disks, as well as differences which suggest an additional role of stellar migration and/or gas accretion in the growth of disk galaxies with an outer up-bending profile, as expected from theoretical models. |
- |
dc.identifier.bibliographicCitation |
IAU Symposium- Formation and Evolution of Galaxy Outskirts, pp.163 - 171 |
- |
dc.identifier.doi |
10.1017/s1743921316011479 |
- |
dc.identifier.uri |
https://scholarworks.unist.ac.kr/handle/201301/53362 |
- |
dc.publisher |
IAU |
- |
dc.title |
The MAD View on the Outskirts of Disks |
- |
dc.type |
Conference Paper |
- |
dc.date.conferenceDate |
2016-03-14 |
- |