The HI mass function in Ursa Major
| dc.creator | Verheijen, Marc | |
| dc.creator | Trentham, Neil | |
| dc.creator | Tully, Brent | |
| dc.creator | Zwaan, Martin | |
| dc.date | 2000-06-08 | |
| dc.date.accessioned | 2026-07-07T01:53:55Z | |
| dc.date.available | 2026-07-07T01:53:55Z | |
| dc.description | A deep blind HI survey of the nearby spiral rich Ursa Major cluster has been performed with the VLA in parallel with a wide-field R-band imaging campaign of most VLA fields with the CFHT. The goal is to measure the slope of the HI mass function down to HI masses of 10^7 Msun as well as the slope of the faint-end of the luminosity function down to M(R)=-10. The VLA survey sampled 16% of the Ursa Major cluster volume. Both the HIMF and the LF in Ursa Major are nearly flat at their faint-ends. No free- floating HI clouds were detected. | |
| dc.description | 7 pages, 3 figures. Contribution to the Guanajuato meeting "Mapping the Hidden Universe". To appear in PASP, 2000 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0006122 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0006122 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/1144 | |
| dc.subject | Astrophysics | |
| dc.title | The HI mass function in Ursa Major | |
| dc.type | text |