This research aims to understand how mass is distributed in the solar neighborhood using pulsar acceleration.
Measured the acceleration of pulsars in the Galaxy
Analyzed data to map mass distribution
Utilized information about stellar remnants
Found varying mass distributions in different areas of the solar neighborhood
Mapped the locations and densities of pulsars to show mass effects
Resumen
Weighing Our Solar NeighborhoodMeasuring the acceleration of stellar remnants called pulsars helps researchers map how mass is distributed in our region of the Galaxy.