Effective temperatures,radii, and luminosities of O emission,Be and Ae stars |
| |
| Authors: | Jong-Ok Woo |
| |
| Institution: | (1) Department of Earth Science, Pusan National University, Pusan, Korea |
| |
| Abstract: | Our de-reddened fluxes, together with the ultraviolet measurements of Thompsonet al. (1978), have been compared with those of Kurucz's (1979) model atmospheres to derive effective temperatures of some O emission, Be and Ae stars. With the measured monochromatic fluxes we determined their angular diameters and luminosities. It is found that the majority of the stars are cooler than the Zero-Age Main Sequence (ZAMS), suggesting that they are slightly more evolved than ZAMS stars.Paper presented at the IAU Third Asian-Pacific Regional Meeting, held in Kyoto, Japan, between 30 September–6 October, 1984. The observations were made at the Observatoire de Haute Provence (France) and La Silla (E.S.O., Chile). |
| |
| Keywords: | |
| 本文献已被 SpringerLink 等数据库收录！ |
|
