DISK OF Be STAR WITH EMISSION
Autor: | Dae-Gun Ahn, Jang-Ho Bae, Sang-Gak Lee, Yeon-Gyung Ko, Suk-Chul Kang, Young-Woo Shin |
---|---|
Rok vydání: | 2007 |
Předmět: |
Physics
Be star K-type main-sequence star Astrophysics::Instrumentation and Methods for Astrophysics Astronomy Astrophysics::Cosmology and Extragalactic Astrophysics General Medicine Astrophysics Herbig Ae/Be star Self guided Spectral line law.invention Telescope Stars law Astrophysics::Solar and Stellar Astrophysics Astrophysics::Earth and Planetary Astrophysics Spectrograph Astrophysics::Galaxy Astrophysics |
Zdroj: | Publications of The Korean Astronomical Society. 22:133-140 |
ISSN: | 1225-1534 |
DOI: | 10.5303/pkas.2007.22.4.133 |
Popis: | We have determined the disk size of Be stars by using emission. We observed spectra of Be stars with telescope in SNU, equipped with SB SGS (Santa Babara Self Guided Spectrograph) and CCD ST-8. The size of disk of Be stars was estimated with the Be star model of Grundstrom & Gies (2006). This study suggests that the medium resolution spectra taken with small telescope equipped with commercial spectrograph are useful to estimate the approximate size of the emitting disk around Be stars. |
Databáze: | OpenAIRE |
Externí odkaz: |