Pith. sign in

REVIEW

The magnetic characteristics of Galactic OB stars from the MiMeS survey of magnetism in massive stars

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1310.3965 v1 pith:6GNI3L6B submitted 2013-10-15 astro-ph.SR

The magnetic characteristics of Galactic OB stars from the MiMeS survey of magnetism in massive stars

G.A. Wade , J. Grunhut , E. Alecian , C. Neiner , M. Auriere , D.A. Bohlender , A. David-Uraz , C. Folsom
show 6 more authors
H.F. Henrichs O. Kochukhov S. Mathis S. Owocki V. Petit the MiMeS Collaboration
This is my paper
classification astro-ph.SR
keywords starsmagnetismmassivemimescharacteristicsgalacticprojectsurvey
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

The Magnetism in Massive Stars (MiMeS) project represents the largest systematic survey of stellar magnetism ever undertaken. Based on a sample of over 550 Galactic B and O-type stars, the MiMeS project has derived the basic characteristics of magnetism in hot, massive stars. Herein we report preliminary results.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.