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Abstract <p>The magnetic field structures of the primary components in threeclose binary systems have been studied. In all their properties,they do not differ from single magnetic stars. There are signsthat the rotational momentum is lost in two ways: 1)&#xa0;it istransferred to the clouds surrounding the magnetic protostar alongthe field lines and 2)&#xa0;through tidal interactions with a closecomponent. Within the hypothesis of the fossil origin of magneticstars, a possible scheme for the formation of close binary systemswith a magnetic companion has been considered.</p>

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Structure of Magnetic Fields of Primary Components of Close Binary Systems BD\(-\)19 5044L, HD 37017, HD 98088

  • 期刊论文

  • 发表日期：

    2025年9月1日

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  • Yu. V. Glagolevskij

摘要

Abstract

The magnetic field structures of the primary components in threeclose binary systems have been studied. In all their properties,they do not differ from single magnetic stars. There are signsthat the rotational momentum is lost in two ways: 1) it istransferred to the clouds surrounding the magnetic protostar alongthe field lines and 2) through tidal interactions with a closecomponent. Within the hypothesis of the fossil origin of magneticstars, a possible scheme for the formation of close binary systemswith a magnetic companion has been considered.