Early-type Galaxy Halo Dynamics inferred using the PN Spectrograph
| dc.creator | Douglas, N. G. | |
| dc.creator | Romanowsky, A. J. | |
| dc.creator | Kuijken, K. | |
| dc.creator | Merrifield, M. R. | |
| dc.creator | Napolitano, N. R. | |
| dc.creator | Arnaboldi, M. | |
| dc.creator | Freeman, K. C. | |
| dc.creator | Capaccioli, M. | |
| dc.creator | Gerhard, O. | |
| dc.date | 2003-10-31 | |
| dc.date.accessioned | 2026-07-07T02:10:58Z | |
| dc.date.available | 2026-07-07T02:10:58Z | |
| dc.description | A new instrument is providing crucial data with which to probe the structure of dark halos in elliptical galaxies. | |
| dc.description | Poster presentation, written contribution for proceedings | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0310900 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0310900 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/6920 | |
| dc.subject | Astrophysics | |
| dc.title | Early-type Galaxy Halo Dynamics inferred using the PN Spectrograph | |
| dc.type | text |