This happens due to a nearby stars matter being pulled towards the neutron star.Thanks for your help with the name....Tom Science 4
2006-12-09 11:46:27 · 6 answers · asked by Anonymous in Science & Mathematics ➔ Astronomy & Space
Gravitational Collapse. The internal outward pressure is no longer able to combat the force of the inward pulling gravity and gravitational collpase insues.
Once the mass of the Star has collapsed beyond the Schwarzschild radius, then you've got a (non-rotating) Black Hole. When speaking of Neutron Stars and Black Holes it's important to also introduce Chandrasekhars limit which specifies which stars will collapse into Neutron Stars, and will lead inevitably to Black Holes (Tolman-Oppenheimer-Volkoff limit) due to inherent gravitational instability.
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2006-12-09 12:00:10 · answer #1 · answered by mytraver 3 · 1⤊ 0⤋
One probability could be in case you had a binary equipment the place neither famous guy or woman on my own substitute into huge sufficient to style a black hollow, and one famous guy or woman collapsed right into a neutron famous guy or woman, which then began "consuming" or gravitationally soaking up the mass from its better half famous guy or woman. finally all of the greater mass will conquer the electron degeneracy, and then the NEUTRON degeneracy, and what you finally end up with is the degenerate mass, possibly in basic terms a set or quarks or bosons, which, of direction, have an get away velocity greater beneficial than C. The neutrons dont "fuse" they give way into their element factors. Theres greater than a number of empty area interior a neutron, iTs regularly electrostatic repulsion between quarks.
2016-12-18 10:34:11 · answer #2 · answered by ? 4 · 0⤊ 0⤋
The process where matter is drawn off one star onto another is called Roche Lobe Overflow. This explains some novae and a group of stars called cataclysmic variables, but I'm not sure that black holes have been formed that way. If they did, they'd be overcoming neutron degeneracy pressure.
2006-12-10 00:14:54 · answer #3 · answered by Iridflare 7 · 0⤊ 0⤋
The Chandrasekar limit is the mass at which a white dwarf (not a neutron star) collapses.
Oh, and check out SS433...
2006-12-09 12:21:07 · answer #4 · answered by grotereber 3 · 0⤊ 0⤋
Hi. You already have it. Collapse.
2006-12-09 11:48:43 · answer #5 · answered by Cirric 7 · 0⤊ 0⤋
implosion
2006-12-09 11:48:49 · answer #6 · answered by Anonymous · 0⤊ 0⤋