This is the first neutron star in which an extended signal has been seen only in infrared light. The remarkable discovery was made by a team of international researchers who have offered two possible explanations for the extended infrared signal – a dusty disk or an energetic wind known as a pulsar wind.
Scientists observed an extended area of infrared emissions around this particular neutron star, which belongs to a group of seven nearby X-ray pulsars — nicknamed ‘the Magnificent Seven.’
Lead author of the study Bettina Posselt said one possible explanation is that there is a disk of material – most likely dust – surrounding the pulsar.
“Such a disk would be composed of matter from the progenitor massive star. Its subsequent interaction with the neutron star could have heated the pulsar and slowed its rotation,” Posselt said.
This phenomenon is known as supernova fallback disk, and if confirmed as the source of the signal it could change our general understanding of neutron star evolution, according to Posselt.
Another theory is that the emission was caused by a pulsar wind slamming into the neutron star as it sped through interstellar space. The shocked particles would then emit synchrotron radiation, causing the extended infrared signal that we see. read more…