3XMM J004232.1+411314
3XMM J004232.1+411314 is a low-mass X-ray binary hosted in the galaxy M31. This object is notable for being the most luminous source of hard X-rays in the Andromeda Galaxy. This is also the most luminous source known that shows dips in the X-ray light curve. The compact object in this system has been unambiguously identified as a neutron star with a spin period of 3 seconds.
Link from a Wikipage to another Wikipage
primaryTopic
3XMM J004232.1+411314
3XMM J004232.1+411314 is a low-mass X-ray binary hosted in the galaxy M31. This object is notable for being the most luminous source of hard X-rays in the Andromeda Galaxy. This is also the most luminous source known that shows dips in the X-ray light curve. The compact object in this system has been unambiguously identified as a neutron star with a spin period of 3 seconds.
has abstract
3XMM J004232.1+411314 is a low ...... th a spin period of 3 seconds.
@en
Link from a Wikipage to an external page
Wikipage page ID
58,535,063
page length (characters) of wiki page
Wikipage revision ID
982,703,830
Link from a Wikipage to another Wikipage
colwidth
constell
epoch
J2000.0
@en
wikiPageUsesTemplate
comment
3XMM J004232.1+411314 is a low ...... th a spin period of 3 seconds.
@en
label
3XMM J004232.1+411314
@en