other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
2018MNRAS.478.3506C - Mon. Not. R. Astron. Soc., 478, 3506-3512 (2018/August-2)
Not an oxymoron: some X-ray binary pulsars with enormous spin-up rates reveal weak magnetic fields.
CHRISTODOULOU D.M., LAYCOCK S.G.T. and KAZANAS D.
Abstract (from CDS):
Abstract Copyright: © 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): accretion, accretion discs - stars: neutron - stars: pulsars: individual: (SXP1062, SXP1323, NGC 300 ULX1) - magnetic fields - X-rays: binaries
Simbad objects: 7
To bookmark this query, right click on this link: simbad:2018MNRAS.478.3506C and select 'bookmark this link' or equivalent in the popup menu