Observational Properties of Primordial Stellar Populations
| dc.creator | Panagia, N. | |
| dc.creator | Stiavelli, M. | |
| dc.creator | Ferguson, H. C. | |
| dc.creator | Stockman, H. S. | |
| dc.date | 2002-09-13 | |
| dc.date.accessioned | 2026-07-07T02:05:10Z | |
| dc.date.available | 2026-07-07T02:05:10Z | |
| dc.description | We present the first results of a study of the expected properties of the first stellar generations in the Universe. In particular, we consider and discuss a series of properties that, on the basis of the emission from associated HII regions, permit one to discern {\it bona fide} primeval stellar generations from the ones formed after pollution from supernova explosions. The expected performance of NGST for the study and the characterization of primordial sources is also discussed. | |
| dc.description | 5 pages, 7 figures. To appear in the proceedings of the Conference 'Galaxy Evolution: Theory and Observations', Cozumel (Mexico), 8-12 April 2002, Eds. V. Avila-Reese, C. Firmani, C. Frenk, & C. Allen, RevMexAA SC (2002) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0209278 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0209278 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/5021 | |
| dc.subject | Astrophysics | |
| dc.title | Observational Properties of Primordial Stellar Populations | |
| dc.type | text |