Of?p stars: a class of slowly rotating magnetic massive stars
classification
🌌 astro-ph.SR
keywords
magneticstarsbeenfieldsclasscharacteristicsconfiningdense
pith:CR6V3VZ3 Add to your LaTeX paper
What is a Pith Number?\usepackage{pith}
\pithnumber{CR6V3VZ3}
Prints a linked pith:CR6V3VZ3 badge after your title and writes the identifier into PDF metadata. Compiles on arXiv with no extra files. Learn more
read the original abstract
Only 5 Of?p stars have been identified in the Galaxy. Of these, 3 have been studied in detail, and within the past 5 years magnetic fields have been detected in each of them. The observed magnetic and spectral characteristics are indicative of organised magnetic fields, likely of fossil origin, confining their supersonic stellar winds into dense, structured magnetospheres. The systematic detection of magnetic fields in these stars strongly suggests that the Of?p stars represent a general class of magnetic O-type stars.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.