Free Access

This article has an erratum: [https://doi.org/10.1051/0004-6361/201731519e]


Fig. 1

image

Rotation period versus its time derivative (“P- diagram”) for all known neutron stars. Lines of constant spin-down rate are shown and labeled. The small dark blue and medium light amber dots denote the known neutron stars not in our database, and the neutron stars in our database with no detected glitches, respectively. The large orange and turquoise dots represent those pulsars in our database with large glitches, and only small glitches detected, respectively. The turquoise triangles correspond to the magnetars in our database, which only have small glitches detected. P and for neutron stars not in our database were taken from the ATNF pulsar catalog 2 (Manchester et al. 2005).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.