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In recent years Herbig Ae/Be stars receive considerable attention as their disks are believed to be the sites of on-going planet formation. Confirming the presence of magnetic fields in these stars is critical for understanding the…

Solar and Stellar Astrophysics · Physics 2019-08-14 S. P. Järvinen , T. A. Carroll , S. Hubrig , I. Ilyin , M. Schöller

To investigate statistically whether magnetic fields in massive stars are ubiquitous or appear in stars with specific spectral classification, certain ages, or in a special environment, we acquired 41 new spectropolarimetric observations…

While several observational investigations have revealed the presence of magnetic fields in the circumstellar envelopes, jets and outflows of post-Asymptotic Giant Branch stars (PAGBs) and planetary nebulae (PNe), none has clearly…

Solar and Stellar Astrophysics · Physics 2015-06-23 L. Sabin , G. A. Wade , A. Lèbre

We present here the final results of the first spectropolarimetric survey of a small sample of active M dwarfs, aimed at providing observational constraints on dynamo action on both sides of the full-convection threshold (spectral type M4).…

Solar and Stellar Astrophysics · Physics 2010-06-28 J. Morin , J. F. Donati , P. Petit , X. Delfosse , T. Forveille , M. M. Jardine

We focus on early-B type stars with helium overabundance, for which the presence of a magnetic field has not previously been reported. The measurements were carried out using high-spectral-resolution spectropolarimetric observations…

Solar and Stellar Astrophysics · Physics 2018-10-10 S. P. Järvinen , S. Hubrig , I. Ilyin , M. Schöller , M. -F. Nieva , N. Przybilla , N. Castro

It is essential for the understanding of stellar structure models of high mass stars to explain why constant stars, non-pulsating chemically peculiar hot Bp stars and pulsating stars co-exist in the slowly pulsating B stars and beta Cephei…

Astrophysics · Physics 2009-11-11 M. Briquet , S. Hubrig , M. Schoeller , P. De Cat

In the context of the MiMeS survey of magnetism in massive stars, 85 classical Be stars were observed in circular polarization with the aim of detecting magnetic fields at their surfaces. No direct evidence of such fields is found, in…

Solar and Stellar Astrophysics · Physics 2014-11-25 G. A. Wade , V. Petit , J. Grunhut , C. Neiner

Context. In chemically peculiar Ap/Bp stars with large-scale organised magnetic fields with a simple centred dipole configuration, the ratio between the maximum and the minimum of the mean magnetic field modulus is of the order of 1.25.…

Solar and Stellar Astrophysics · Physics 2024-05-21 S. Hubrig , S. D. Chojnowski , S. P. Jarvinen , I. Ilyin , K. Pan

We have investigated a sample of 28 well-known spectroscopically-identified magnetic Ap/Bp stars, with weak, poorly-determined or previously undetected magnetic fields, with the aim of exploring the weak part of the magnetic field…

To understand the origin of the magnetic fields in massive stars as well as their impact on stellar internal structure, evolution, and circumstellar environment, within the MiMeS project, we searched for magnetic objects among a large…

In this article, we present the results of an analysis of chemical abundances and a search for magnetic fields in eight field blue horizontal-branch (BHB) stars: BD\,+01$^{\circ}$0548, HD\,74721, HD\,86986, HD\,87112, HD\,93329, HD\,109995,…

Solar and Stellar Astrophysics · Physics 2025-09-23 Issouf Kafando , Gregg Wade , Alexandre David-Uraz , Francis LeBlanc , Carmelle Robert

Observations of magnetic fields of stars at the pre-main sequence phase can provide important new insights into the complex physics of the late stages of star formation. This is especially true at intermediate stellar masses, where magnetic…

Solar and Stellar Astrophysics · Physics 2009-01-21 G. A. Wade , E. Alecian , J. Grunhut , C. Catala , S. Bagnulo , C. P. Folsom , J. D. Landstreet

With this work, we have conducted an extensive search for magnetic fields in the photosphere of $\alpha$~And. We have acquired new circular polarisation spectra with the MuSiCoS and ESPaDOnS sp ectropolarimeters. We have also obtained FORS1…

We present the results of a magnetic survey with FORS1 in polarimetric mode of a sample of B and Herbig Ae stars with previously undetected magnetic fields. For the first time a mean longitudinal magnetic field at a level higher than 3…

Astrophysics · Physics 2007-05-23 S. Hubrig , T. Szeifert , P. North , M. Schoeller , R. V. Yudin

We present the results of the continuation of our magnetic survey with FORS1 at the VLT of a sample of B-type stars consisting of confirmed or candidate beta Cephei stars and Slowly Pulsating B (hereafter SPB) stars, along with a small…

Solar and Stellar Astrophysics · Physics 2009-11-13 S. Hubrig , M. Briquet , P. De Cat , M. Schoeller , T. Morel , I. Ilyin

Our recent discovery of magnetic fields in a small number of Herbig Ae/Be stars has required that we survey a much larger sample of stars. From our FORS1 and ESPaDOnS surveys, we have acquired about 125 observations of some 70 stars in…

The number of magnetic stars detected among massive stars is small; nevertheless, the role played by the magnetic field in stellar evolution cannot be disregarded. Links between line profile variability, enhancements/depletions of surface…

Fossil magnetic fields of early-type stars are typically characterised by symmetric or slightly distorted oblique dipolar surface geometries. Contrary to this trend, the late-B magnetic chemically peculiar star HD 57372 exhibits an…

Solar and Stellar Astrophysics · Physics 2025-04-30 Oleg Kochukhov

Our knowledge of the presence and the strength of magnetic fields in intermediate-mass pre-main-sequence stars remains very poor. We present new magnetic field measurements in six Herbig Ae/Be stars observed with HARPS in…

Solar and Stellar Astrophysics · Physics 2015-06-16 S. Hubrig , I. Ilyin , M. Schoeller , G. Lo Curto

We present the analysis performed on spectropolarimetric data of 97 O-type targets included in the framework of the MiMeS (Magnetism in Massive Stars) Survey. Mean Least-Squares Deconvolved Stokes I and V line profiles were extracted for…