The Star-formation History of the Universe
| dc.creator | Rowan-Robinson, M. | |
| dc.date | 1999-06-18 | |
| dc.date.accessioned | 2026-07-07T02:32:05Z | |
| dc.date.available | 2026-07-07T02:32:05Z | |
| dc.description | The star formation history derived from ultraviolet and H$α$ data, without correction for dust extinction, on the one hand, and from far infrared and submillimetre data, on the other, is investigated. The latter estimates are found to be a factor 2-3 higher than the former, consistent with 2/3-3/4 of the uv light in star forming regions being absorbed by dust and reemitted in the far infrared. A reanalysis of the Hubble Deep Field galaxies using photometric reshifts shows no evidence for a decline in star formation rate at z = 2-4. A simple and versatile parameterized approach to the star formation history allows a quantitative investigation of the constraints from far infrared and submillimetre counts and background intensity measurements. A good fit to the counts, the 850 $μ$m background and the star formation history can be found in an $Ω_o$ = 1 universe, but this model fails to account for even the lowest estimates of the 140-350 $μ$m background by a factor of 2. Either the observed values are overestimated or we need a new population of found in a $Λ$ = 0, $Ω_o$ = 0.3 universe. | |
| dc.description | 10 pages, 7 figures, to appear in proceedings of the Ringberg Workshop on 'Ultraluminous galaxies: Monsters or Babies ?', 1999, eds D.Lutz and L.Tacconi, Astrophys.Space Sci., in press | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9906308 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9906308 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/14387 | |
| dc.subject | Astrophysics | |
| dc.title | The Star-formation History of the Universe | |
| dc.type | text |