Dark matter heats up in dwarf galaxies. Issue 1 (3rd January 2019)
- Record Type:
- Journal Article
- Title:
- Dark matter heats up in dwarf galaxies. Issue 1 (3rd January 2019)
- Main Title:
- Dark matter heats up in dwarf galaxies
- Authors:
- Read, J I
Walker, M G
Steger, P - Abstract:
- ABSTRACT: Gravitational potential fluctuations driven by bursty star formation can kinematically 'heat up' dark matter at the centres of dwarf galaxies. A key prediction of such models is that, at a fixed dark matter halo mass, dwarfs with a higher stellar mass will have a lower central dark matter density. We use stellar kinematics and HI gas rotation curves to infer the inner dark matter densities of eight dwarf spheroidal and eight dwarf irregular galaxies with a wide range of star formation histories. For all galaxies, we estimate the dark matter density at a common radius of 150 pc, $\rho _{\rm DM}(150\, \mathrm{pc})$ . We find that our sample of dwarfs falls into two distinct classes. Those that stopped forming stars over 6 Gyr ago favour central densities $\rho _{\rm DM}(150\, \mathrm{pc})\gt 10^8$ M⊙ kpc −3, consistent with cold dark matter cusps, while those with more extended star formation favour $\rho _{\rm DM}(150\, \mathrm{pc})\lt 10^8$ M⊙ kpc −3, consistent with shallower dark matter cores. Using abundance matching to infer pre-infall halo masses, M 200, we show that this dichotomy is in excellent agreement with models in which dark matter is heated up by bursty star formation. In particular, we find that $\rho _{\rm DM}(150\, \mathrm{pc})$ steadily decreases with increasing stellar mass-to-halo mass ratio, M * / M 200 . Our results suggest that, to leading order, dark matter is a cold, collisionless, fluid that can be kinematically 'heated up' and movedABSTRACT: Gravitational potential fluctuations driven by bursty star formation can kinematically 'heat up' dark matter at the centres of dwarf galaxies. A key prediction of such models is that, at a fixed dark matter halo mass, dwarfs with a higher stellar mass will have a lower central dark matter density. We use stellar kinematics and HI gas rotation curves to infer the inner dark matter densities of eight dwarf spheroidal and eight dwarf irregular galaxies with a wide range of star formation histories. For all galaxies, we estimate the dark matter density at a common radius of 150 pc, $\rho _{\rm DM}(150\, \mathrm{pc})$ . We find that our sample of dwarfs falls into two distinct classes. Those that stopped forming stars over 6 Gyr ago favour central densities $\rho _{\rm DM}(150\, \mathrm{pc})\gt 10^8$ M⊙ kpc −3, consistent with cold dark matter cusps, while those with more extended star formation favour $\rho _{\rm DM}(150\, \mathrm{pc})\lt 10^8$ M⊙ kpc −3, consistent with shallower dark matter cores. Using abundance matching to infer pre-infall halo masses, M 200, we show that this dichotomy is in excellent agreement with models in which dark matter is heated up by bursty star formation. In particular, we find that $\rho _{\rm DM}(150\, \mathrm{pc})$ steadily decreases with increasing stellar mass-to-halo mass ratio, M * / M 200 . Our results suggest that, to leading order, dark matter is a cold, collisionless, fluid that can be kinematically 'heated up' and moved around. … (more)
- Is Part Of:
- Monthly notices of the Royal Astronomical Society. Volume 484:Issue 1(2019)
- Journal:
- Monthly notices of the Royal Astronomical Society
- Issue:
- Volume 484:Issue 1(2019)
- Issue Display:
- Volume 484, Issue 1 (2019)
- Year:
- 2019
- Volume:
- 484
- Issue:
- 1
- Issue Sort Value:
- 2019-0484-0001-0000
- Page Start:
- 1401
- Page End:
- 1420
- Publication Date:
- 2019-01-03
- Subjects:
- galaxies: dwarf -- galaxies: haloes -- galaxies: kinematics and dynamics -- galaxies: star formation -- cosmology: observations -- dark matter
Astronomy -- Periodicals
Periodicals
520.5 - Journal URLs:
- http://mnras.oxfordjournals.org/ ↗
http://onlinelibrary.wiley.com/journal/10.1111/(ISSN)1365-2966 ↗
http://www.blackwell-synergy.com/issuelist.asp?journal=mnr ↗
http://www.blackwell-synergy.com/loi/mnr ↗
http://ukcatalogue.oup.com/ ↗ - DOI:
- 10.1093/mnras/sty3404 ↗
- Languages:
- English
- ISSNs:
- 0035-8711
- Deposit Type:
- Legaldeposit
- View Content:
- Available online (eLD content is only available in our Reading Rooms) ↗
- Physical Locations:
- British Library DSC - 5943.000000
British Library DSC - BLDSS-3PM
British Library HMNTS - ELD Digital store - Ingest File:
- 11977.xml