2021MNRAS.500.1992T


Query : 2021MNRAS.500.1992T

2021MNRAS.500.1992T - Mon. Not. R. Astron. Soc., 500, 1992-1999 (2021/January-2)

The complex fossil magnetic field of the δ Scuti star HD 41641.

THOMSON-PARESSANT K., NEINER C., ZWINTZ K. and ESCORZA A.

Abstract (from CDS):

Only three magnetic δ Scuti stars are known as of today. HD 41641 is a δ Scuti star showing chemical peculiarities and rotational modulation of its light curve, making it a good magnetic candidate. We acquired spectropolarimetric observations of this star with NARVAL at Telescope Bernard Lyot (TBL) to search for the presence of a magnetic field and characterize it. We indeed clearly detect a magnetic field in HD 41641, making it the fourth known magnetic δ Scuti star. Our analysis shows that the field is of fossil origin, like magnetic OBA stars, but with a complex field structure rather than the much more usual dipolar structure.

Abstract Copyright: © 2020 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): stars: chemically peculiar - stars: individual: HD 41641 - stars: magnetic field - stars: oscillations - stars: variables: Scuti

Status at CDS : Large table(s) will be appraised for possible ingestion in VizieR.

Simbad objects: 7

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Number of rows : 7
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 * bet Cas dS* 00 09 10.68518 +59 08 59.2120 2.73 2.61 2.27 1.97 1.77 F2III 551 0
2 V* CP Oct dS* 03 09 53.7500021592 -83 31 53.581689012   8.01 7.61     F2/3Ib/II 66 0
3 HD 35929 Ae* 05 27 42.7906489200 -08 19 38.446702140   8.55 8.11     F2IV/V 125 0
4 V* V901 Ori Ro* 05 40 56.3704617744 -01 30 25.856677224 5.96 6.82 6.96     B2V 354 2
5 HD 41641 dS* 06 06 40.5782639808 +06 43 49.884406824   8.14 7.86     A5III 32 0
6 * rho Pup dS* 08 07 32.6488235 -24 18 15.567946 3.43 3.24 2.81 2.46 2.25 F5IIkF2IImF5II 322 0
7 HD 188774 dS* 19 55 10.0375808184 +41 17 10.271172480   9.05 8.81     A9IV 43 0

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