Torna ai risultati
Scheda bibliografica · Consultazione e accesso
Artículo

The globular cluster kinematics and galaxy dark matter content of NGC 3923

Norris, Mark A. et al · Wiley · 2012

Testo completo ad accesso aperto
Lettura rapida. Controlla i dati essenziali della risorsa e accedi al contenuto con il pulsante principale. La scheda mostra solo le informazioni necessarie per identificare, citare e aprire l’opera.

Accesso alla risorsa

Apri il contenuto dall’opzione principale o scegli un’altra fonte disponibile.

CONICET Digital CONICET Digital OAI-PMH
Entrar por CONICET Digital
Accesso principale

Testo completo ad accesso aperto

Texto completo identificado como acceso abierto.
Apri testo

Riepilogo

Descripción general del contenido del recurso.

This paper presents further results from our spectroscopic study of the globular cluster (GC) system of the group elliptical NGC 3923. From observations made with the GMOS instrument on the Gemini South telescope, an additional 50 GC and Ultra Compact Dwarf (UCD) candidates have been spectroscopically confirmed as members of the NGC 3923 system. When the recessional velocities of these GCs are combined with the 29 GC velocities reported previously, a total sample of 79 GC/UCD velocities is produced. This sample extends to over 6 arcmin (>6 Re ∼30 kpc) from the centre of NGC 3923, and is used to study the dynamics of the GC system and the dark matter content of NGC 3923. It is found that the GC system of NGC 3923 displays no appreciable rotation, and that the projected velocity dispersion is constant with radius within the uncertainties. The velocity dispersion profiles of the integrated light and GC system of NGC 3923 are indistinguishable over the region in which they overlap. We find some evidence that the diffuse light and GCs of NGC 3923 have radially biased orbits within ∼130′′. The application of axisymmetric orbit-based models to the GC and integrated light velocity dispersion profiles demonstrates that a significant increase in the mass-to-light ratio (from M/LV = 8 to 26) at large galactocentric radii is required to explain this observation. We therefore confirm the presence of a dark matter halo in NGC 3923. We find that dark matter comprises 17.5+7.3 −4.5% of the mass within 1 Re, 41.2+18.2 −10.6% within 2 Re, and 75.6+15.4 −16.8% within the radius of our last kinematic tracer at 6.9 Re. The total dynamical mass within this radius is found to be 1.5+0.4 −0.25×1012 M⊙. In common with other studies of large ellipticals, we find that our derived dynamical mass profile is consistently higher than that derived by X-ray observations, by a factor of around 2. Fil: Norris, Mark A. . University Of Durham; Reino Unido Fil: Gebhardt, Karl . University of Texas; Estados Unidos

Come citare

Elegí el formato que necesitás y copiá la referencia al portapapeles.

APA 7

Norris, M. A. E. A. (2012). The globular cluster kinematics and galaxy dark matter content of NGC 3923. http://hdl.handle.net/11336/15038

MLA

Norris, Mark A. et al. "The globular cluster kinematics and galaxy dark matter content of NGC 3923." 2012. http://hdl.handle.net/11336/15038.

Chicago

Norris, Mark A. et al. 2012. "The globular cluster kinematics and galaxy dark matter content of NGC 3923.". http://hdl.handle.net/11336/15038.

Harvard

Norris, M. A. E. A. 2012, The globular cluster kinematics and galaxy dark matter content of NGC 3923, Wiley, available at: http://hdl.handle.net/11336/15038 [Accessed 7 Aug. 2026].

Condividi e stampa

Salva la scheda, copia il link permanente o stampala in PDF.

Esporta riferimento

Esporta il record nei formati più comuni per usarlo con un gestore bibliografico.

Dettagli della risorsa

Informazioni bibliografiche utili per verificare che sia il materiale corretto.

Titolo
The globular cluster kinematics and galaxy dark matter content of NGC 3923
Autore / collaboratori
Norris, Mark A. et al
Editore
Wiley
Anno di pubblicazione
2012
ISSN
1485-1498
ISSN
1485-1498
Lingua
Inglés

Soggetti

Esplora risorse correlate a partire da questi soggetti.

Copiato