Magnetic Fields of Chemically Peculiar and Related Stars. VIII. Main Results of 2021 and Near-Future Prospects [PDF]
Astrophysical Bulletin, 2022 —We present a review of the papers written in the research field of stellar magnetism in 2021. The instruments, observation, and data analysis methods, photometry, spectroscopy, and spectropolarimetry results are considered.
Romanyuk I.
europepmc +2 more sources
The Surface Composition of Six Newly Discovered Chemically Peculiar Stars. Comparison to the HgMn Stars mu Lep and beta Scl and the Superficially Normal B Star nu Cap [PDF]
Astronomical Journal, 2023 We report on a detailed abundance study of six bright, mostly southern, slowly rotating late B-stars: HD 1279 (B8III), HD 99803 (B9V), HD 123445 (B9V), HD 147550 (B9V), HD 171961 (B8III), and HD 202671 (B5II/III), hitherto reported as normal stars.
R. Monier +12 more
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Photometric variability of the LAMOST sample of magnetic chemically peculiar stars as seen by TESS [PDF]
Astronomy & Astrophysics, 2023 High-quality light curves from space missions have opened up a new window on the rotational and pulsational properties of magnetic chemically peculiar (mCP) stars and have fuelled asteroseismic studies. They allow the internal effects of surface magnetic
J. Labadie-Bartz +4 more
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Analysis of eight magnetic chemically peculiar stars with rotational modulation [PDF]
Monthly notices of the Royal Astronomical Society, 2022 Since the end of 2018, the Transiting Exoplanet Survey Satellite (TESS) has provided stellar photometry to the astronomical community. We have used TESS data to study rotational modulation in the light curves of a sample of chemically peculiar stars ...
O. Kobzar +11 more
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The detection of magnetic chemically peculiar stars using Gaia BP/RP spectra [PDF]
Astronomy & Astrophysics, 2022 The magnetic chemically peculiar (mCP) stars of the upper main sequence are perfectly suited to studying the effects of rotation, diffusion, mass-loss, accretion, and pulsation in the presence of an organized stellar magnetic field.
E. Paunzen, M. Prišegen
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Spectropolarimetry of Magnetic Chemically Peculiar Stars in the Orion OB1 Association [PDF]
, 2022 We summarise the results of a spectropolarimetric survey of 56 chemically peculiar (CP) stars in the association of Orion OB1. We uniformly collected the observational material with the 6-m telescope BTA of the Special Astrophysical Observatory in 2013 ...
E. Semenko +4 more
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Chemically Peculiar Stars in the Open Cluster Stock 2 [PDF]
Astronomical Journal, 2022 The recently rediscovered open cluster Stock 2, located roughly 375 pc away and about 400 Myr old, has the potential to be an exciting new testbed for our understanding of stellar evolution.
L. Casamiquela +4 more
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High-resolution spectroscopic analysis of four new chemically peculiar stars [PDF]
, 2022 We present detailed chemical compositions of four stars on the first-ascent red giant branch that are classified as chemically peculiar, but lack comprehensive analyses at high spectral resolution.
M. Roriz +5 more
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Twenty-year monitoring of the surface magnetic fields of chemically peculiar stars [PDF]
Monthly notices of the Royal Astronomical Society, 2021 Magnetic chemically peculiar stars of the main sequence can present rotational periods as long as many decades. Here we report the results of an observational campaign started in 2001 aimed at establishing these very long periods from the variability ...
M. Giarrusso +7 more
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Chemically Peculiar Stars in Integrated Light Stellar Population Models and Local Group Galaxies [PDF]
, 2022 Integrated-light models that incorporate common types of chemically peculiar (CP) stars are assembled using synthetic spectra. Selected spectral features encode significant age information for populations with ages $\sim$50 Myr $
G. Worthey, Xiang-dong Shi
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