HB morphology and the Second Parameter Effect: Faint Stars in a big game
| dc.creator | Pecci, Flavio Fusi | |
| dc.creator | Bellazzini, Michele | |
| dc.date | 1997-01-07 | |
| dc.date.accessioned | 2026-07-07T02:22:40Z | |
| dc.date.available | 2026-07-07T02:22:40Z | |
| dc.description | We schematically review some of the main steps in the study of the Horizontal Branch Morphology in Galactic Globular Clusters. Since the first realization of the existence of the so-called Second Parameter Problem (2nd-P) up to now, one could perhaps see a sort of circular path. Actually, many candidate 2nd-P's were proposed during the early '70s, age has been the top-scored 2nd-P during the late '80s, and we are now back to even more candidates, including also possible intriguing combinations of some of them. | |
| dc.description | AASlatex, 9 pages, no figures - Invited Review presented at the Third Conference on Faint Blue Stars, Schenectady (NY), october 14-17, 1996 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9701026 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9701026 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/10957 | |
| dc.subject | Astrophysics | |
| dc.title | HB morphology and the Second Parameter Effect: Faint Stars in a big game | |
| dc.type | text |