Recent observations have revealed the structural properties of the dark and luminous mass distribution in spirals. These results led to the vision of a new and amazing scenario. The investigation of single and coadded objects has shown that the rotation curves of spirals follow, from their centers out to their virial radii, an universal profile that implies a tuned combination of their stellar disk and dark halo mass distributions. This, alongside with accurate mass modeling of individual galaxies, poses important challenges to the presently theoretically favored ΛCDM Cosmology.
Dark matter in galaxies: Leads to its nature / Salucci, P.; De Laurentis, M.. - In: POS PROCEEDINGS OF SCIENCE. - ISSN 1824-8039. - 161:(2013), pp. 1-10. (Intervento presentato al convegno VIII International Workshop on the Dark Side of the Universe tenutosi a Rio de Janeiro nel 10th to 15th June, 2012) [10.22323/1.161.0012].
Dark matter in galaxies: Leads to its nature
Salucci, P.;
2013-01-01
Abstract
Recent observations have revealed the structural properties of the dark and luminous mass distribution in spirals. These results led to the vision of a new and amazing scenario. The investigation of single and coadded objects has shown that the rotation curves of spirals follow, from their centers out to their virial radii, an universal profile that implies a tuned combination of their stellar disk and dark halo mass distributions. This, alongside with accurate mass modeling of individual galaxies, poses important challenges to the presently theoretically favored ΛCDM Cosmology.| File | Dimensione | Formato | |
|---|---|---|---|
|
DSU 2012_012.pdf
accesso aperto
Tipologia:
Versione Editoriale (PDF)
Licenza:
Creative commons
Dimensione
629.92 kB
Formato
Adobe PDF
|
629.92 kB | Adobe PDF | Visualizza/Apri |
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
