SRVs in the Solar Neighbourhood
| dc.creator | Glass, I. S. | |
| dc.date | 2006-09-18 | |
| dc.date.accessioned | 2026-07-07T07:23:15Z | |
| dc.date.available | 2026-07-07T07:23:15Z | |
| dc.description | Period-luminosity sequences have been shown to exist among the Semi-Regular Variables (SRVs) of the Magellanic Clouds (Wood et al, 1999), the Bulge of the Milky Way galaxy (Glass & Schultheis, 2003) and elsewhere. It would clearly be useful to have absolute (trigonometric) calibrations of these relations. This paper investigates whether the sequences can be seen among the M-type giant SRVs of the solar neighbourhood. Mass loss phenomena among these stars and their dependence on period and spectral sub-type are also discussed. | |
| dc.description | 2 pages, 3 figures | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0609482 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0609482 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/115916 | |
| dc.subject | Astrophysics | |
| dc.title | SRVs in the Solar Neighbourhood | |
| dc.type | text |