No CrossRef data available.
Article contents
Fitting of Silicon lines in UV and Balmer Hδ Line in Optical Spectra of B supergiant HD 198478
Published online by Cambridge University Press: 23 April 2012
Abstract
Atmospheric parameters of the Galactic early B-supergiant HD 198478 (55 Cyg) were determined from the UV silicon lines and optical Balmer Hδ 4101 Å line. TLUSTY synthetic spectra were broadened using the ROTIN numerical code in order to determine effective temperature, surface gravity, rotational and macroturbulent velocity.
- Type
- Contributed Papers
- Information
- Copyright
- Copyright © International Astronomical Union 2012