On the incidence of magnetic fields in slowly-pulsating B, Beta Cephei and B-type emission line stars
arXiv:0906.1575 · doi:10.1111/j.1365-2966.2009.15208.x
Abstract
We have obtained 40 high-resolution circular spectropolarimetric measurements of 12 slowly-pulsating B (SPB) stars, 8 Beta Cephei stars and two Be stars with the ESPaDOnS and NARVAL spectropolarimeters. The aim of these observations is to evaluate recent claims of a high incidence of magnetic field detections in stars of these types obtained using low-resolution spectropolarimetry by Hubrig (2006), Hubrig (2007) and Hubrig (2009). The precision achieved is generally comparable to or superior to that obtained by Hubrig et al., although our new observations are distinguished by their resolution of metallic and He line profiles, and their consequent sensitivity to magnetic fields of zero net longitudinal component. In the SPB stars we confirm the detection of magnetic field in one star (16 Peg), but find no evidence of the presence of fields in the remaining 11. In the Beta Cep stars, we detect a field in xi^1 CMa, but not in any of the remaining 7 stars. Finally, neither of the two B-type emission line stars shows any evidence of magnetic field. Based on our results, we conclude that fields are not common in SPB, Beta Cep and B-type emission line stars, consistent with the general rarity of fields in the broader population of main sequence B-type stars.
Accepted - MNRAS
References in corpus (7)
- Discovery of magnetic fields in the beta Cephei star xi^1 CMa and in several Slowly Pulsating B stars
- Characterisation of the magnetic field of the Herbig Be star HD 200775
- Discovery of two magnetic massive stars in the Orion Nebula Cluster: a clue to the origin of neutron star magnetic fields?
- New magnetic field measurements of beta Cephei stars and Slowly Pulsating B stars
- Discovery of magnetic fields in the very young, massive stars W601 (NGC 6611) and OI 201 (NGC 2244)
- Attempts to measure the magnetic field of the pulsating B star Eridani
- Evidence for weak magnetic fields in early-type emission stars
Cited by in corpus (45)
- Classical Be Stars: Rapidly Rotating B Stars with Viscous Keplerian Decretion Disks
- A high-resolution spectropolarimetric survey of Herbig Ae/Be stars - I. Observations and measurements
- A Magnetic Confinement vs. Rotation Classification of Massive-Star Magnetospheres
- The MiMeS Survey of Magnetism in Massive Stars: Introduction and overview
- Magnetic field measurements and their uncertainties: the FORS1 legacy
- Early magnetic B-type stars: X-ray emission and wind properties
- B fields in OB stars (BOB): low-resolution FORS2 spectropolarimetry of the first sample of 50 massive stars
- Fundamental properties of nearby single early B-type stars
- NGC 1624-2: A slowly rotating, X-ray luminous Of?cp star with an extraordinarily strong magnetic field
- Detection of a magnetic field on HD108: clues to extreme magnetic braking and the Of?p phenomenon
- The surface nitrogen abundance of a massive star in relation to its oscillations, rotation, and magnetic field
- Revisiting the Rigidly Rotating Magnetosphere model for sigma Ori E. I. Observations and Data Analysis
- HR 5907: Discovery of the most rapidly rotating magnetic B-type star by the MiMeS Collaboration
- Systematic detection of magnetic fields in massive, late-type supergiants
- MOBSTER -- VI. The crucial influence of rotation on the radio magnetospheres of hot stars
- Discovery of a magnetic field in the O9 sub-giant star HD 57682 by the MiMeS Collaboration
- Magnetic fields in massive stars, their winds, and their nebulae
- Discovery of a strong magnetic field in the rapidly rotating B2Vn star HR 7355
- The importance of non-photon noise in stellar spectropolarimetry. The spurious detection of a non-existing magnetic field in the A0 supergiant HD 92207
- Magnetic field detection in the B2Vn star HR 7355
- Are there tangled magnetic fields on HgMn stars?
- Critical evaluation of magnetic field detections reported for pulsating B-type stars in the light of ESPaDOnS, Narval and reanalyzed FORS1/2 observations
- Discovery of the magnetic field in the pulsating B star beta Cephei
- Analytical maximum likelihood estimation of stellar magnetic fields
- B fields in OB stars (BOB): on the detection of weak magnetic fields in the two early B-type stars beta CMa and epsilon CMa
- The surface magnetic field and chemical abundance distributions of the B2V helium-strong star HD184927
- The pulsating magnetosphere of the extremely slowly rotating magnetic Cep star CMa
- CoRoT high-precision photometry of the B0.5 IV star HD 51756
- Bayesian inference of solar and stellar magnetic fields in the weak-field approximation
- Statistics of Magnetic Fields for OB Stars
- The B Fields in OB Stars (BOB) Survey
- An Observational Evaluation of Magnetic Confinement in the Winds of BA Supergiants
- Discovery of a magnetic field in the early B-type star sigma Lupi
- gamma Peg: testing Vega-like magnetic fields in B stars
- Weak magnetic field, solid-envelope rotation, and wave-induced N-enrichment in the SPB star Cassiopeiae
- Period change and stellar evolution of Cephei stars
- Confirmation of xi^1 CMa's ultra-slow rotation: magnetic polarity reversal and a dramatic change in magnetospheric UV emission lines
- Be Stars: Rapidly Rotating Pulsators
- Magnetic fields in O-, B- and A-type stars on the main sequence
- The magnetic field of the stripped primary in the upsilon Sgr system, a member of the rare class of hydrogen-deficient binaries
- Observations of magnetic fields in hot stars
- On the use of the first-order moment approach for measurements of H_eff from LSD profiles
- An observer's view on the future of asteroseismology
- Analytical calculation of Stokes profiles of rotating stellar magnetic dipole
- CMa: An Extremely Slowly Rotating Magnetic B0.7 IV Star