Towards using optical/NIR photometry to measure the temperature of O stars
| dc.creator | Apellániz, J. Maíz | |
| dc.creator | Sota, A. | |
| dc.date | 2007-02-20 | |
| dc.date.accessioned | 2026-07-07T07:47:39Z | |
| dc.date.available | 2026-07-07T07:47:39Z | |
| dc.description | It has been traditionally stated that it is not possible to use optical/NIR photometry to measure the temperatures of O stars. In this contribution we describe the steps required to overcome the hurdles that have prevented this from happening in the past and we present our preliminary results for the low-extinction case. | |
| dc.description | 2 pages, to appear in Massive Stars: Fundamental Parameters and Circumstellar Interactions | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0702516 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0702516 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/124241 | |
| dc.subject | Astrophysics | |
| dc.title | Towards using optical/NIR photometry to measure the temperature of O stars | |
| dc.type | text |