Magnetic Field of the Solar-Like Star β Aql: a Study by Individual Spectral Lines
Abstract
We present the results of the spectropolarimetric study of the solar-like star β Aql in individual spectral lines. The magnetic field on β Aql was detected with maximal value B =19.7 ±2.8 G, and minimal value B =-18.1 ±3.5 G. We suppose a difference in magnetic field value measured using spectral lines with normal and anomalous Zeeman spleeting.
- Publication:
-
Stars: From Collapse to Collapse
- Pub Date:
- June 2017
- Bibcode:
- 2017ASPC..510..251B