2017AstBu..72..411G


Query : 2017AstBu..72..411G

2017AstBu..72..411G - Astrophys. Bull., 72, 411-417 (2017/December-0)

Three three-dipole stars.

GLAGOLEVSKIJ Y.V. and NAZARENKO A.F.

Abstract (from CDS):

We analyzed magnetic-field structures of three three-dipole magnetic stars HD 18078, HD 37776, and HD 149438. The fact that the model and observed phase dependences B_e and B_s for HD 18078 computed with the same parameters of the dipoles agree with each other shows conclusively that global magnetic structures are formed by dipole structures. Magnetic poles show up conspicuously on Mercator maps of the distribution of magnetic field, the field strength there is maximal and equal to B_p = 3577, 10 700, and 275 G in the three stars mentioned above.Dipole modelsmake it possible to analyze magnetic-field structure inside stars.

Abstract Copyright: ∼

Journal keyword(s): stars: magnetic field - stars: individual: (HD 18078, HD 37776, HD 149438)

Status at CDS : Objects in title, abstract, text, figures, and all or part of small table(s) being processed in SIMBAD.

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 HD 18078 a2* 02 56 32.0098959576 +56 10 41.434633848   8.50 8.27     A0pSrCr 96 0
2 V* V901 Ori Ro* 05 40 56.3704617744 -01 30 25.856677224 5.96 6.82 6.96     B2V 354 2
3 * tau Sco * 16 35 52.9528530 -28 12 57.661515 1.55 2.56 2.81 2.93 3.18 B0V 959 0

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