Interaction between dark matter sub-halos and a galactic gaseous disk
We investigate the idea that the interaction of dark matter (DM) sub-halos with the gaseous disks of galaxies can be the origin for the observed holes and shells found in their neutral hydrogen (H I ) distributions. We use high-resolution hydrodynamic simulations to show that pure DM sub-halos impac...
Gespeichert in:
| Hauptverfasser: | , |
|---|---|
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2012 January 19
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| In: |
The astrophysical journal
Year: 2012, Jahrgang: 746, Heft: 1, Pages: 1-8 |
| ISSN: | 1538-4357 |
| DOI: | 10.1088/0004-637X/746/1/10 |
| Online-Zugang: | Verlag, Volltext: http://dx.doi.org/10.1088/0004-637X/746/1/10 Verlag, Volltext: http://stacks.iop.org/0004-637X/746/i=1/a=10 
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| Verfasserangaben: | Rahul Kannan, Andrea V. Macciò, Anna Pasquali, Benjamin P. Moster, Fabian Walter |
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