| dc.creator |
Shabani, F |
|
| dc.creator |
Grebel, EK |
|
| dc.creator |
Pasquali, A |
|
| dc.creator |
D'Onghia, E |
|
| dc.creator |
III, GJS |
|
| dc.creator |
Adamo, A |
|
| dc.creator |
Messa, M |
|
| dc.creator |
Elmegreen, BG |
|
| dc.creator |
Dobbs, C |
|
| dc.creator |
Gouliermis, DA |
|
| dc.creator |
Calzetti, D |
|
| dc.creator |
Grasha, K |
|
| dc.creator |
Elmegreen, DM |
|
| dc.creator |
Cignoni, M |
|
| dc.creator |
Dale, DA |
|
| dc.creator |
Aloisi, A |
|
| dc.creator |
Smith, LJ |
|
| dc.creator |
Tosi, M |
|
| dc.creator |
Thilker, DA |
|
| dc.creator |
Lee, JC |
|
| dc.creator |
Sabbi, E |
|
| dc.creator |
Kim, H |
|
| dc.creator |
Pellerin, A |
|
| dc.date |
2018-11-23T15:26:12Z |
|
| dc.date |
2018-05-16 |
|
| dc.date |
2018-11-23T15:26:12Z |
|
| dc.date.accessioned |
2022-05-27T01:03:16Z |
|
| dc.date.available |
2022-05-27T01:03:16Z |
|
| dc.identifier |
Vol. 478, pp. 3590 - 3604 |
|
| dc.identifier |
10.1093/mnras/sty1277 |
|
| dc.identifier |
http://hdl.handle.net/10871/34890 |
|
| dc.identifier |
0035-8711 |
|
| dc.identifier |
Monthly Notices of the Royal Astronomical Society |
|
| dc.identifier.uri |
http://localhost:8080/xmlui/handle/CUHPOERS/241936 |
|
| dc.description |
This is the final version. Available from OUP via the DOI in this record |
|
| dc.description |
One of the main theories for explaining the formation of spiral arms in galaxies is the stationary density wave theory. This theory predicts the existence of an age gradient across the arms. We use the stellar cluster catalogues of the galaxies NGC 1566, M51a, and NGC 628 from the Legacy ExtraGalactic UV Survey (LEGUS) program. In order to test for the possible existence of an age sequence across the spiral arms, we quantified the azimuthal offset between star clusters of different ages in our target galaxies. We found that NGC 1566, a grand-design spiral galaxy with bisymmetric arms and a strong bar, shows a significant age gradient across the spiral arms that appear to be consistent with the prediction of the stationary density wave theory. In contrast, M51a with its two well-defined spiral arms and a weaker bar does not show an age gradient across the arms. In addition, a comparison with non-LEGUS star cluster catalogues for M51a yields similar results. We believe that the spiral structure of M51a is not the result of a stationary density wave with a fixed pattern speed. Instead, tidal interactions could be the dominant mechanism for the formation of spiral arms. We also found no offset in the azimuthal distribution of star clusters with different ages across the weak spiral arms of NGC 628. |
|
| dc.description |
This work is based on observations made with the NASA/ESA HST, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with program 13364. Support for Program 13364 was provided by NASA through a grant from the Space Telescope Science Institute.
This research has made use of the NED, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.
AA acknowledges the support of the Swedish Research Council (Vetenskapsrådet) and the Swedish National Space Board. DAG kindly acknowledges financial support by the German Research Foundation (DFG) through programme GO 1659/3-2. |
|
| dc.language |
en |
|
| dc.publisher |
Oxford University Press (OUP) / Royal Astronomical Society |
|
| dc.rights |
© 2018 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved |
|
| dc.subject |
galaxies: individual: NGC 1566, M51, NGC 628 |
|
| dc.subject |
galaxies: spiral |
|
| dc.subject |
galaxies: structure |
|
| dc.title |
Search for star cluster age gradients across spiral arms of three LEGUS disc galaxies |
|
| dc.type |
Article |
|