The stellar orbit distribution in present-day galaxies inferred from the CALIFA survey
The distribution of circularity of stellar orbits within 300 galaxies of the present-day Universe, with masses between 108.7 and 1011.9 M ⊙, is directly observed by the CALIFA survey and provides a benchmark for galaxy simulations.
Gespeichert in:
| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
01 January 2018
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| In: |
Nature astronomy
Year: 2018, Jahrgang: 2, Heft: 3, Pages: 233-238 |
| ISSN: | 2397-3366 |
| DOI: | 10.1038/s41550-017-0348-1 |
| Online-Zugang: | Verlag, Volltext: http://dx.doi.org/10.1038/s41550-017-0348-1 Verlag, Volltext: https://www.nature.com/articles/s41550-017-0348-1 
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| Verfasserangaben: | Ling Zhu, Glenn van de Ven, Remco van den Bosch, Hans-Walter Rix, Mariya Lyubenova, Jesús Falcón-Barroso, Marie Martig, Shude Mao, Dandan Xu, Yunpeng Jin, Aura Obreja, Robert J.J. Grand, Aaron A. Dutton, Andrea V. Macciò, Facundo A. Gómez, Jakob C. Walcher, Rubén García-Benito, Stefano Zibetti, Sebastian F. Sánchez |
| Zusammenfassung: | The distribution of circularity of stellar orbits within 300 galaxies of the present-day Universe, with masses between 108.7 and 1011.9 M ⊙, is directly observed by the CALIFA survey and provides a benchmark for galaxy simulations. |
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| Beschreibung: | Gesehen am 19.03.2018 |
| Beschreibung: | Online Resource |
| ISSN: | 2397-3366 |
| DOI: | 10.1038/s41550-017-0348-1 |