Polarized X-ray and optical emission from PSR J1023+0038 are aligned and match the pulsed flux spectrum, pointing to synchrotron radiation at a pulsar wind-disk shock as the emission mechanism.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.HE 1years
2024 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Polarized multiwavelength emission from pulsar wind - accretion disk interaction in a transitional millisecond pulsar
Polarized X-ray and optical emission from PSR J1023+0038 are aligned and match the pulsed flux spectrum, pointing to synchrotron radiation at a pulsar wind-disk shock as the emission mechanism.