2012MNRAS.420.2727E


Query : 2012MNRAS.420.2727E

2012MNRAS.420.2727E - Mon. Not. R. Astron. Soc., 420, 2727-2735 (2012/March-1)

Magnetic stars from a FEROS cool Ap star survey.

ELKIN V.G., KURTZ D.W. and NITSCHELM C.

Abstract (from CDS):

New magnetic Ap stars with split Zeeman components are presented. These stars were discovered from observations with the Fibre-fed Extended Range Optical Spectrograph (FEROS) spectrograph at the European Southern Observatory (ESO) 2.2-m telescope. 15 new magnetic stars are analysed here. Several stars with very strong magnetic fields were found, including HD 70702 with a 15-kG magnetic field strength, and HD 168767 with a 16.5-kG magnetic field strength measured using split Zeeman components of spectral lines and by comparison with synthetic calculations. The physical parameters of the stars were estimated from photometric and spectroscopic data. Together with previously published results for stars with strong magnetic fields, the relationship between magnetic field strength and rotation period is discussed.

Based on observations collected at the European Southern Observatory, La Silla, Chile, as part of programmes 078.D-0080(A), 080.D- 0191(A), 081.D-2002(A), 082.D-0061(A), 083.D-0034(A) and 084.D-0067(A).


Abstract Copyright: 2012 The Authors Monthly Notices of the Royal Astronomical Society2012 RAS

Journal keyword(s): techniques: spectroscopic - stars: chemically peculiar - stars: magnetic field - stars: variables: general

Simbad objects: 19

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Number of rows : 19
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 3988 SB* 00 39 15.3393329208 -83 01 58.520691228   8.51 8.35     ApCrEu 23 0
2 HD 21336 * 03 26 36.6311005440 +05 29 19.431744936   9.57 9.28     A2 9 0
3 NGC 2244 334 Y*O 06 32 51.7919732079 +04 47 16.160568228 13.17 13.38 12.95 12.46 12.34 B5V 48 0
4 HD 57040 a2* 07 16 42.2413712736 -53 26 13.116548076   9.76 9.24     A(pEuSr) 19 0
5 HD 61513 * 07 38 27.4642819896 -30 03 48.675293856   10.16 10.11     ApCrEuSr 11 0
6 HD 70702 * 08 21 00.8179235640 -51 32 36.847901400   8.56 8.57     ApEuCrSr 12 0
7 HD 75049 a2* 08 45 33.0714336288 -50 43 58.323425736   9.09 9.14     ApEuCr 36 0
8 HD 76460 * 08 53 08.3801914008 -62 26 42.137312892   10.18 9.80     ApSr 17 0
9 HD 81588 * 09 24 54.4141546032 -48 29 07.357356492   8.72 8.45     ApSrCrEu 32 0
10 HD 88241 SB* 10 09 27.5324278320 -40 28 26.415262236   8.95 8.59     ApSr(EuCr) 27 0
11 HD 158450 ** 17 29 43.9848254928 -08 01 03.169337592   8.91 8.55     ApSi(Cr) 42 0
12 HD 162316 a2* 17 59 07.9447174536 -75 47 55.666197492   9.79 9.36     ApSrEu(Cr) 13 0
13 HD 168767 * 18 22 30.3413564928 -26 54 40.347424980   8.88 8.71 9.499   ApEuCr(Sr) 12 0
14 HD 177268 * 19 05 25.6965714504 -34 16 28.288334820   9.21 9.14     ApCrEu 12 0
15 HD 179902 * 19 15 08.1441567120 -21 44 15.135815472   10.35 10.07     A0III 11 0
16 HD 184120 ** 19 33 39.2413 -20 28 51.470   10.44 10.37 10.45   ApEuCr 11 0
17 HD 185204 * 19 40 06.2820810096 -46 54 26.703334188   9.95 9.53     ApSrEuCr 12 0
18 HD 191695 * 20 12 02.5031386080 -21 18 02.809847052   10.24 9.86     ApSrEu(Cr) 24 0
19 V* GL Lac a2* 22 44 07.5047456400 +55 35 21.211012248   8.85 8.82     kB9hB7HeB8pSi 293 0

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