Paper:	Magnetic Field of the Solar-Like Star β Aql: a Study by Individual Spectral Lines
Volume:	510, Stars: From Collapse to Collapse
Page:	251
Authors:	Butkovskaya, V. V.; Plachinda, S. I.; Baklanova, D. N.; Pankov, N. F.
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.

Astronomical Society of the Pacific
Conference Series

© Copyright 1988 - 2024 - Astronomical Society of the Pacific
No part of the material protected by this copyright may be reproduced or used in any form other than for personal use without written permission from the ASP.

Page generated in 0.078 seconds