On Properties of Main Sequence Magnetic Stars

  title={On Properties of Main Sequence Magnetic Stars},
  author={Yu. V. Glagolevskij},
  journal={Astrophysical Bulletin},
We reconsidered the previous studies of properties of magnetic stars based on the latest data on average surface magnetic fields of 177 stars. New, corrected results have been obtained that allow a better understanding of the phenomenon of magnetic chemically peculiar stars. 
8 Citations
Secular Stability of the Magnetic Structures of Magnetic Stars. II
Numerous indications that the magnetic field structures in magnetic stars do not change with age are cited. The stars rotate like a solid.
Remarks on Difference of Properties of Am and Ap Stars
We performed the comparative analysis of the properties of Ap and Am stars. It is shown that the main differences in the formation and evolution of these objects are due to the influence of a
Characteristics of Magnetic Star Formation at the Early Stages of Evolution
Abstract —The results of works dedicated to the study of the early stages of evolution of magnetic and non-magnetic chemically peculiar stars are discussed. The fossil hypothesis of the formation of
Remarks on the Properties of the Magnetic Field of the Star HD37776
Studies of the magnetic field and its structure in the star HD37776 by various authors are discussed. Significant conflicts among these results are noted which suggest that the star has not been
Secular Stability of Magnetic Field Structures in Magnetic CP-Stars
The magnetic field structures of stars with different ages are studied. No changes in the position and orientation of magnetic dipoles with age are observed. It is concluded that there are no global
Evolutionary Features and Other Characteristics of Magnetic Stars with Helium Anomalies (He-r, He-w)
Abstract —We critically review the results of earlier studies on magnetic stars with anomalous helium lines. We discuss the issues associated with the fossil-field theory and the scenario of the
Magnetic Fields of Chemically Peculiar and Related Stars. VI. Main Results of 2019 and Near-Future Prospects
We present a review of the papers written in the field of stellar magnetism studies in 2020. More than 70 original papers related to different areas of the specified scientific topics have been
Benchmarking the fundamental parameters of Ap stars with optical long-baseline interferometric measurements
Context. The variety of physical processes at play in chemically peculiar stars makes it difficult to determine their fundamental parameters. In particular, for the magnetic ones, called Ap stars,


Progress in Studies of the Evolution of the Magnetic Fields of CP-Stars. I
In this review (part I) the most important results of research on the properties of the magnetic fields of chemically peculiar stars prior to 2000 are examined critically. The properties of the
Investigations of the Magnetic Fields of Chemically Peculiar Stars of Different Age
1. The program of comprehensive investigations of stellar magnetism in the Special Astrophysical Observatory of the USSR AS includes the study of origin and evolution of the stellar magnetic fields
Evolution of the Magnetic Fields of Main-Sequence CP-Stars. IV
A possible scenario is proposed for the origin and evolution of magnetic stars based on the observational data accumulated up to now. The large difference in magnetic structures and the predominant
Magnetic Stars After the Hayashi Phase. II.
The properties of magnetic stars derived from observational data are analyzed. The degree of “magnetic” braking of parent protostars, which depends the magnetic field and mass, is studied. The
Evolutionary state of magnetic chemically peculiar stars
Context. The photospheres of about 5–10% of the upper main sequence stars exhibit remarkable chemical anomalies. Many of these chemically peculiar (CP) stars have a global magnetic field, the origin
General properties of magnetic CP stars
We present the review of our previous studies related to observational evidence of the fossil field hypothesis of formation and evolution of magnetic and non-magnetic chemically peculiar stars.
Effective temperature of Ap and Am stars from Geneva photometry
The determination of the effective temperature of different kinds of chemically peculiar stars from Geneva photometry is rediscussed. We propose an improved method of determining T eff of Ap stars
Evolution of the magnetic fields of main-sequence CP-stars. I.
A study of the average surface magnetic fields Bs shows that the damping time for the magnetic field of chemically peculiar stars is τ ~ 108 −109 years, which is consistent with the assumption of
Fundamental stellar parameters derived from the evolutionary tracks
The surface gravities and radii of stars are calculated for different MK spectral types using the masses of stars determined from their evolutionary tracks in the HR diagram and the most reliable
Evolution of the Magnetic Fields of Main-Sequence CP-Stars. V
The rate of magnetic field relaxation in magnetic CP-stars after they emerge from the zero age Main-sequence line is discussed. Data are introduced which indicate a slow increase in the large-scale