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相关论文: Discovery of kilogauss magnetic fields in three DA…

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We have detected longitudinal magnetic fields between 2 and 4kG in three normal DA white dwarfs (WD0446-790, WD1105-048, WD2359$-$434) out of a sample of 12 by using optical spectropolarimetry done with the VLT Antu 8 m telescope equipped…

天体物理学 · 物理学 2007-05-23 R. Aznar Cuadrado , S. Jordan , R. Napiwotzki , H. M. Schmid , S. K. Solanki , G. Mathys

Context: About 10% of white dwarfs have magnetic fields with strength in the range between about 10^5 and 3x10^8 G. It is not known whether the remaining white dwarfs are not magnetic, or if they have a magnetic field too weak to be…

太阳与恒星天体物理 · 物理学 2015-06-11 J. D. Landstreet , S. Bagnulo , G. G. Valyavin , L. Fossati , S. Jordan , D. Monin , G. Wade

Weak magnetic field has been searched for on only a small number of white dwarfs. Current estimates for white dwarfs with fields in excess of 1MG are about 10%; according to previous studies this number increases up to about 25% in the kG…

天体物理学 · 物理学 2007-05-23 S. Jordan , R. Aznar Cuadrado , R. Napiwotzki , H. M. Schmid , S. K. Solanki

Magnetic fields are present in roughly 10% of white dwarfs. These fields affect the structure and evolution of such stars, and may provide clues about their earlier evolution history. Particularly important for statistical studies is the…

太阳与恒星天体物理 · 物理学 2019-03-06 John D. Landstreet , Stefano Bagnulo

We present new results of a survey for weak magnetic fields among DA white dwarfs with inclusion of some brighter hot subdwarf stars. We have detected variable circular polarization in the Halpha line of the hot subdwarf star Feige 34 (SP:…

天体物理学 · 物理学 2008-11-26 G. Valyavin , S. Bagnulo , S. Fabrika , A. Reisenegger , G. A. Wade , Inwoo Han , D. Monin

Current estimates for white dwarfs with fields in excess of 1MG are about 10%; according to our first high-precision circular-polarimetric study of 12 bright white dwarfs with the VLT (Aznar Cuadrado et al. 2004) this number increases up to…

天体物理学 · 物理学 2007-05-23 S. Jordan , R. Aznar Cuadrado , R. Napiwotzki , H. M. Schmid , S. K. Solanki

We have carried out a re-analysis of polarimetric data of central stars of planetary nebulae, hot subdwarfs, and white dwarfs taken with FORS1 (FOcal Reducer and low dispersion Spectrograph) on the VLT (Very Large Telescope), and added a…

太阳与恒星天体物理 · 物理学 2012-10-16 S. Jordan , S. Bagnulo , J. Landstreet , L. Fossati , G. G. Valyanin , D. Monin , G. A. Wade , K. Werner , S. J. O'Toole

We report the discovery of weak magnetic fields in three white dwarfs within the local 20pc volume (WD 0816-310, WD 1009-184, and WD 1532+129), and we confirm the magnetic nature of a fourth star (WD 2138-332) in which we had previously…

太阳与恒星天体物理 · 物理学 2019-09-25 S. Bagnulo , J. D. Landstreet

Many stars evolve into magnetic white dwarfs, and observations may help to understand when the magnetic field appears at the stellar surface, if and how it evolves during the cooling phase, and what are the mechanisms that generate it.…

太阳与恒星天体物理 · 物理学 2021-10-04 S. Bagnulo , J. D. Landstreet

Magnetic fields are detected in a few percent of white dwarfs. The number of such magnetic white dwarfs known is now some hundreds. Fields range in strength from a few kG to several hundred MG. Almost all the known magnetic white dwarfs…

太阳与恒星天体物理 · 物理学 2017-11-22 J. D. Landstreet , S. Bagnulo , G. Valyavin , A. F. Valeev

Our knowledge of the magnetism in white dwarfs is based on an observational dataset that is biased in favour of stars with very strong magnetic fields. Most of the field measurements available in the literature have a relatively low…

太阳与恒星天体物理 · 物理学 2018-10-24 Stefano Bagnulo , John D. Landstreet

This paper describes results of magnetic field measurements of white dwarfs carried out on the 6-m telescope for the last years. A magnetic field of about Be ~ 28 kG has been discovered in the degenerate star WD 1953-011. A rotational…

天体物理学 · 物理学 2007-05-23 S. N. Fabrika , G. G. Valyavin , T. E. Burlakova , E. A. Barsukova , D. N. Monin

Searches for magnetic fields in white dwarfs have clarified both the frequency of occurrence and the global structure of the fields found down to field strengths of the order of 500 kG. Below this level, the situation is still very unclear.…

太阳与恒星天体物理 · 物理学 2015-08-19 J. D. Landstreet , S. Bagnulo , G. G. Valyavin , D. Gadelshin , A. J. Martin , G. Galazutdinov , E. Semenko

We report the discovery of a new magnetic DA white dwarf (WD), WD0011-721, which is located within the very important 20pc volume-limited sample of the closest WDs to the Sun. This star has a mean field modulus <|B|> of 343 kG, and from the…

太阳与恒星天体物理 · 物理学 2019-08-07 John D. Landstreet , Stefano Bagnulo

A significant fraction of white dwarfs harbour a magnetic field with strengths ranging from a few kG up to about 1000 MG. The fraction appears to depend on the specific class of white dwarfs being investigated and may hold some clues to the…

太阳与恒星天体物理 · 物理学 2018-01-18 A. Kawka

A significant fraction of white dwarfs possess a magnetic field with strengths ranging from a few kG up to about 1000 MG. However, the incidence of magnetism varies when the white dwarf population is broken down into different spectral…

太阳与恒星天体物理 · 物理学 2020-10-14 Adela Kawka

Isolated magnetic white dwarfs have field strengths ranging from kilogauss to gigagauss, and constitute an interesting class of objects. The origin of the magnetic field is still the subject of a hot debate. Whether these fields are fossil,…

太阳与恒星天体物理 · 物理学 2016-02-17 Enrique García-Berro , Mukremin Kilic , S. O. Kepler

Magnetic fields have been detected in several hundred white dwarfs, with strengths ranging from a few kG to several hundred MG. Only a few of the known fields have a mean magnetic field modulus below about 1 MG. We are searching for new…

太阳与恒星天体物理 · 物理学 2016-06-29 J. D. Landstreet , S. Bagnulo , A. Martin , G. Valyavin

Fifty-two magnetic white dwarfs have been identified in spectroscopic observations from the Sloan Digital Sky Survey (SDSS) obtained between mid-2002 and the end of 2004, including Data Releases 2 and 3. Though not as numerous nor as…

The sample of white dwarfs included in the local 20 pc volume documents, fairly accurately, the total production of white dwarfs over roughly 10 Gyr of stellar evolution in this part of the Milky Way Galaxy. In this sample, we have been…

太阳与恒星天体物理 · 物理学 2020-11-18 S. Bagnulo , J. D. Landstreet
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