- Abstract:
-
The dark matter (DM) haloes around spiral galaxies appear to conspire with their baryonic content: empirically, significant amounts of DM are inferred only below a universal characteristic acceleration scale. Moreover, the discrepancy between the baryonic and dynamical mass, which is usually interpreted as the presence of DM, follows a very tight mass discrepancy acceleration (MDA) relation. Its universality, and its tightness in spiral galaxies, poses a challenge for the DM interpretation an...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Publisher's version
- Files:
-
-
(pdf, 727.7KB)
-
- Publisher copy:
- 10.1093/mnras/stw1472
-
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- Grant:
- PRIN 2010-2011
- Publisher:
- Oxford University Press Publisher's website
- Journal:
- Monthly Notices of the Royal Astronomical Society Journal website
- Volume:
- 461
- Issue:
- 3
- Pages:
- 2367-2373
- Publication date:
- 2016-06-05
- Acceptance date:
- 2016-06-15
- DOI:
- ISSN:
-
0035-8711 and 1365-2966
- Pubs id:
-
pubs:643749
- URN:
-
uri:7e131775-73de-447d-94b5-268b1bcdcd6d
- UUID:
-
uuid:7e131775-73de-447d-94b5-268b1bcdcd6d
- Local pid:
- pubs:643749
- Copyright holder:
- Cappellari et al
- Copyright date:
- 2016
- Notes:
- © 2016 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal article
The mass discrepancy acceleration relation in early-type galaxies: extended mass profiles and the phantom menace to MOND
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+ Italian Ministry of Education, Universities and Research
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