Beijing-Sana
Chinese astronomers have discovered a non-accumulating, non-radiative neutron star, with a mass about 1.2 times the mass of the sun, using the Lammost Large Sky Region Multi-target Fiber Spectroscopic Telescope.
This discovery will enhance the observation of dense celestial objects such as neutron stars and hard-to-observe black holes, and lead to further study on star formation and evolution, physical properties and formation theory of neutron stars and black holes, Xinhua quoted a study published in the journal Nature Astronomy as saying.
Neutron stars represent dense celestial bodies, formed during the process of the evolution of massive stars until the end of their lives, and finding an appropriate method for observing non-accumulating and non-radiating neutron stars is an important matter for astronomers to study dense celestial bodies.
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