B fields in OB stars (BOB): on the detection of weak magnetic fields in the two early B-type stars<i>β</i> CMa and<i>ϵ</i> CMa
L. Fossati(Austrian Academy of Sciences), H. Sana(Astronomical Institute of the Slovak Academy of Sciences), N. Castro(University of Michigan), F. R. N. Schneider(Jet Propulsion Laboratory), M. Briquet(Centre National de la Recherche Scientifique), T. Morel(University of Liège), T. A. Carroll(Leibniz Institute for Astrophysics Potsdam), I. Ilyin(Leibniz Institute for Astrophysics Potsdam), Andreas Reisenegger(Pontificia Universidad Católica de Chile), A. de Koter(Utrecht University), S. Simón‐Díaz(Universidad de La Laguna), L. M. Oskinova(University of Potsdam), N. Przybilla(University of Bamberg), M. Schöller(European Southern Observatory), S. Hubrig(Leibniz Institute for Astrophysics Potsdam), M. F. Nieva(Friedrich-Alexander-Universität Erlangen-Nürnberg), N. Langer(Netherlands Institute for Radio Astronomy)
Cited by 76
Related Papers
A Massive Pulsar in a Compact Relativistic Binary
|Science|2013|3.8k
How Massive Single Stars End Their Life
|The Astrophysical Journal|2003|2.2k
Binary Interaction Dominates the Evolution of Massive Stars
|Science|2012|2.1k
$\mathsf{\alpha}$-, <i>r</i>-, and <i>s</i>-process element trends in the Galactic thin and thick disks
|Astronomy and Astrophysics|2005|628
An excess of massive stars in the local 30 Doradus starburst
|Science|2018|257