No cores in dark matter-dominated dwarf galaxies with bursty star formation histories
ABSTRACT. Measurements of the rotation curves of dwarf galaxies are often interpreted as requiring a constant density core at the centre, at odds with the ‘cus
Gespeichert in:
| Hauptverfasser: | , , , |
|---|---|
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2019 April 29
|
| In: |
Monthly notices of the Royal Astronomical Society
Year: 2019, Jahrgang: 486, Heft: 4, Pages: 4790-4804 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stz1168 |
| Online-Zugang: | Verlag, Volltext: https://doi.org/10.1093/mnras/stz1168 Verlag, Volltext: https://academic.oup.com/mnras/article/486/4/4790/5481533 
|
| Verfasserangaben: | Sownak Bose, Carlos S. Frenk, Adrian Jenkins, Azadeh Fattahi, Facundo A. Gómez, Robert J.J. Grand, Federico Marinacci, Julio F. Navarro, Kyle A. Oman, Rüdiger Pakmor, Joop Schaye, Christine M. Simpson and Volker Springel |
| Zusammenfassung: | ABSTRACT. Measurements of the rotation curves of dwarf galaxies are often interpreted as requiring a constant density core at the centre, at odds with the ‘cus |
|---|---|
| Beschreibung: | Gesehen am 03.06.2019 |
| Beschreibung: | Online Resource |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stz1168 |