3 papers
astro-ph.HE2026
On the origin of the strong internal magnetic fields of central compact objects
Kazım Yavuz EkÅi, Ä°rem Bakır
Central compact objects are radio-quite young neutron stars associated with supernova remnants. They have relatively small dipole fields, as infer…
astro-ph.HE2026
The period clustering of magnetars and X-ray dim isolated neutron stars
Kazım Yavuz EkÅi
The spin periods of magnetars and X-ray dim isolated neutron stars (XDINS) cluster within a remarkably narrow range. Using the current sample of 30 magnetars with measured periods…
astro-ph.HE2026
Evolution of proto-neutron stars to pulsars, magnetars and central compact objects
Ä°rem Bakır, Kazım Yavuz EkÅi
Some young neutron stars, the magnetars, have ultra-strong magnetic fields, yet their inferred birth rate is comparable to the core-collapse supernova rate, challenging scenarios t…