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Query : 2017MNRAS.471L..96J |
2017MNRAS.471L..96J - Mon. Not. R. Astron. Soc., 471, L96-L100 (2017/October-2)
The relation between stellar magnetic field geometry and chromospheric activity cycles - I. The highly variable field of ε Eridani at activity minimum.
JEFFERS S.V., BORO SAIKIA S., BARNES J.R., PETIT P., MARSDEN S.C., JARDINE M.M. and VIDOTTO A.A.
Abstract (from CDS):
Abstract Copyright: © 2017 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): techniques: polarimetric - stars: activity - stars: individual: ε Eridani - stars: magnetic field - stars: solar-type - stars: solar-type
Simbad objects: 2
Number of rows : 2 |
N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2024 |
#notes |
---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | * eps Eri | BY* | 03 32 55.8444911587 | -09 27 29.739493865 | 5.19 | 4.61 | 3.73 | 3.00 | 2.54 | K2V | 1933 | 1 |
2 | * 61 Cyg A | BY* | 21 06 53.9395895022 | +38 44 57.902349973 | 7.50 | 6.39 | 5.21 | 4.19 | 3.54 | K5V | 1036 | 0 |
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