Astronomers in China have discovered a pulsar that is partially eclipsed by an orbiting companion star in the Milky Way, shedding light on binary star system evolution.
Binary systems involve two stars orbiting each other, with one possibly transferring mass to the other, leading to orbit shrinkage over about 1000 years.
A rare binary system involves a neutron star and a helium star, where the latter can eclipse the former, hindering radio pulse detection from Earth.
Astronomers using FAST in China identified the first such binary system in the Milky Way, named PSR J1928+1815, which has a short spin period.
Observations over 4.5 years showed the system to have an almost circular orbit with a short period of 3.6 hours, during which the companion star eclipses the pulsar.
The system's evolving orbital and spin characteristics suggest significant energy loss, indicating rapid changes.
The discovery confirms long-standing theories on binary star evolution, revealing insights into mass exchange, orbit shrinkage, and neutron star behavior.
This short-lived binary system, lasting 1000 years, demonstrates the common envelope evolution, which is difficult to observe directly.
The system's study presents opportunities to research neutron star matter accretion, cooling processes, and potential future gravitational wave sources.
The findings are detailed in the scientific journal Science, marking a significant astronomical discovery.
This unique observation supports existing theories on binary star system evolution and paves the way for further research and understanding.
The binary pulsar system in the Milky Way could offer valuable insights into the behavior of compact stars and their eventual merger.
The discovery showcases the utility of advanced telescopes like FAST in uncovering rare astronomical phenomena.
Astronomers anticipate that the binary system identified will continue to evolve and ultimately merge, potentially generating gravitational waves.
The study underscores the importance of ongoing astronomical observations in unraveling the mysteries of the cosmos.
The observation of this short-lived binary system provides significant data for astrophysical research and contributes to expanding our knowledge of stellar evolution.