... new insights into the constituents of the galaxy cluster. We know that the microlensing was caused by either a star, a neutron star, or a stellar-mass black hole,” explains Steven Rodney from the University of South Carolina, USA and a co-author...
... and will likely collapse into another type of small dense star known as a neutron star within 10, 000 years. “Its fate will therefore be to undergo core collapse and to form a neutron star,” write the authors in their recent research paper. “Over...
... any evidence for either of these objects yet. To see SN 1987A in all of its glory (minus a black hole or neutron star), the latest visuals can be seen here, here and here (all links open up in a new window). These...
... a similar configuration to HR 6819 or LB-1, but where the inner pair is made up of two black holes or of a black hole and a neutron star. The distant outer object can gravitationally impact the inner pair in such a way that it triggers a merger...
... of the accelerated expansion of the Universe. The appearance of next-generation gravitational wave interferometers has made researching neutron star mergers and black holes possible, whereas medium and large diameter telescopes can find the furthest...
... from x-ray bright binaries. These luminous systems typically contain a neutron star or black hole pulling in gas from a closely orbiting companion star. The material near the neutron star or black hole becomes superheated and shoots off x-rays...