- Abstract:
-
The majority of galaxies in the local Universe exhibit spiral structure with a variety of forms. Many galaxies possess two prominent spiral arms, some have more, while others display a many-armed flocculent appearance. Spiral arms are associated with enhanced gas content and star formation in the discs of low-redshift galaxies, so are important in the understanding of star formation in the local universe. As both the visual appearance of spiral structure, and the mechanisms responsible for it...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Publisher's version
- Files:
-
-
(pdf, 12.0MB)
-
- Publisher copy:
- 10.1093/mnras/stw1588
-
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- Publisher:
- Oxford University Press Publisher's website
- Journal:
- Monthly Notices of the Royal Astronomical Society Journal website
- Volume:
- 461
- Issue:
- 4
- Pages:
- 3663-3682
- Publication date:
- 2016-07-05
- Acceptance date:
- 2016-06-29
- DOI:
- EISSN:
-
1365-2966
- ISSN:
-
0035-8711
- Pubs id:
-
pubs:634445
- URN:
-
uri:51394a1a-fd4e-495a-abcd-e59b0c85e060
- UUID:
-
uuid:51394a1a-fd4e-495a-abcd-e59b0c85e060
- Local pid:
- pubs:634445
- Copyright holder:
- Lintott et al
- Copyright date:
- 2016
- Notes:
- © 2016 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal article
Galaxy Zoo: Comparing the demographics of spiral arm number and a new method for correcting redshift bias
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