binary neutron stars 예문
- :Going by neutron star # Binary neutron stars, yes.
- The formation and evolution of binary neutron stars can be a complex process.
- A subclass of GRBs ( the " short " bursts ) appear to originate from a different process : the merger of binary neutron stars.
- A subclass of GRBs ( the " short " bursts ) appear to originate from a different process, possibly the merger of binary neutron stars.
- Years later, the gleisner Karpal, using a gravitational-wave detector, determines that a binary neutron star system in the constellation of Lacerta has collapsed, releasing a huge burst of energy.
- The true nature of these objects ( or even whether the current classification scheme is accurate ) remains unknown, although the leading hypothesis is that they originate from the mergers of binary neutron stars or a neutron star with a black hole.
- KAGRA will detect chirp waves from binary neutron star coalescence at 240 Fabry-P閞ot cavities, resonant side band extraction method, and so on ) will be extended with an underground location, cryogenic mirrors, and a suspension point interferometer.
- Some evidence gained from analysis of the mass and orbital parameters of binary neutron stars ( which require two such supernovae ) hints that the collapse of an oxygen-neon-magnesium core may produce a supernova that differs observably ( in ways other than size ) from a supernova produced by the collapse of an iron core.