Magnetic Fields of Chemically Peculiar and Related Stars. XI. Main Results Obtained in 2024 and Analysis of Immediate Prospects

This paper presents a review of 67 scientific publications from 2024 devoted to stellar magnetism and related topics. The primary focus of recent research lies in the discovery of new magnetic stars and the monitoring of magnetic fields in chemically peculiar (CP) stars and other stellar types. Interest in the study of magnetic star emission in the X-ray and radio domains has also increased. The most significant new data were obtained using Gaia astrometry, TESS and Kepler photometry, and LAMOST low-resolution spectroscopy. The first results from the new SPIRou and CRIRES+ spectrographs are also discussed.

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Publication Details

Journal
Astrophysical Bulletin
Published
2025-09-01
DOI
https://doi.org/10.1134/s199034132560036x
Primary Topic
Stellar, planetary, and galactic studies
Type
article
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article

Magnetic Fields of Chemically Peculiar and Related Stars. XI. Main Results Obtained in 2024 and Analysis of Immediate Prospects

Astrophysical Bulletin
Stellar, planetary, and galactic studies
article

Magnetic Fields of Chemically Peculiar and Related Stars. XI. Main Results Obtained in 2024 and Analysis of Immediate Prospects

article en

Abstract

This paper presents a review of 67 scientific publications from 2024 devoted to stellar magnetism and related topics. The primary focus of recent research lies in the discovery of new magnetic stars and the monitoring of magnetic fields in chemically peculiar (CP) stars and other stellar types. Interest in the study of magnetic star emission in the X-ray and radio domains has also increased. The most significant new data were obtained using Gaia astrometry, TESS and Kepler photometry, and LAMOST low-resolution spectroscopy. The first results from the new SPIRou and CRIRES+ spectrographs are also discussed.

Astrophysical BulletinVol. 80(3)
Special Astrophysical Observatory (RU)
Openalex Percentile: Top 39%
Stellar, planetary, and galactic studies
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