Magnetic Fields of Chemically Peculiar and Related Stars. 5.Main Results of 2018 and Near-Future Prospects

Discovery of eight 'Main-sequence Radio Pulse emitters' using the GMRT: clues to the onset of coherent radio emission in hot magnetic stars

“…In order to quantify this, we searched the literature for the known magnetic hot stars. The major studies consulted were the following: the studies of Ap, He-weak, and He-strong stars by Borra & Landstreet (1979, 1980; Borra et al (1983) and Bohlender et al (1987Bohlender et al ( , 1993; the slowly rotating Ap star study of Landstreet & Mathys (2000); the study of Ap stars by Aurière et al (2007); the sample of Ap stars in open clusters presented by Landstreet et al (2007Landstreet et al ( , 2008; the Herbig Ae/Be stars studied by Alecian et al (2013); the Of?p stars examined by Petit et al (2013) and Munoz et al (2020); the early B-type stars presented by Shultz et al (2018Shultz et al ( , 2019bShultz et al ( , 2020; the volume-limited sample of Ap stars conducted by Sikora et al (2019b,a); the samples of stars with magnetically split lines examined by Mathys (2017) and Chojnowski et al (2019); and the results of the ongoing survey at the Special Astrophysical Observatory of both field stars (Kudryavtsev et al 2006;Romanyuk et al 2014Romanyuk et al , 2015Romanyuk et al , 2016aRomanyuk et al , 2017aRomanyuk et al , 2018Romanyuk 2019;Romanyuk et al 2020) and stars in the Orion nebula (Romanyuk et al 2016b(Romanyuk et al , 2017b(Romanyuk et al , 2019(Romanyuk et al , 2021. The compilation of longitudinal magnetic field curves provided by Bychkov et al (2020) was also consulted, in order to include magnetic stars reported in single-star papers.…”