1、This is a neutron star.
2、This is the mass of the neutron star m and this is the radius of the neutron star.
3、You always lose your m, and so you find that the speed at which it reaches the neutron star M R M neutron star times G divided by R neutron star.
4、Sometimes a neutron star results and sometimes a black hole.
5、It is the clock of the rotating neutron star.
6、Structure of a pulsar - a rotating magnetic neutron star.
7、For now, I just want to concentrate on this neutron star alone.
8、One teaspoonful of material from a neutron star would weigh a billion tonnes.
9、A thimbleful of a neutron star would weigh over 100 million tons.
10、If the magnetic stress bears up the gravitation in the stellar evolution, the big mass neutron star over the neutron - star mass can not collapse into a black hole.
11、This is when the Duke team had some fun with their laser-trapped neutron star analog.
12、The period of rotation of the neutron star is 0.0335028583 seconds. That's what it is today.
13、It was the first time that astronomers have measured the rate of cooling of a young neutron star.
14、Magnetars are a type of neutron star? An object so dense its protons and electrons have merged to form neutrons.
15、Magnetars are a type of neutron star which has a magnetic field a million billion times stronger than the Earth's.
16、The typical situation involves a loner neutron star that comes a little too close to an ordinary binary pair.
17、A ten-gram object thrown onto a neutron star — the reason being that this velocity becomes enormously high.
18、In theory, the first step toward producing a millisecond pulsar is the formation of a neutron star when a massive star goes supernova.
19、Since a 7-solar-mass is too large to be a white dwarf or neutron star, it must be a black hole.
20、Astarquake is thought to be the tearing apart of the surface of a neutron star, much like an earthquake here on earth.
21、So by timing the pulses of the x-rays, you can get a handle on the Doppler shift of the neutron star.
22、And I take a little bit of matter m, and I drop it from a large distance onto the neutron star.
23、They go around in the plane of the blackboard, say, and so this matter cannot fall radially in but it will fall in and spiral in and forms what we call an accretion disk around the neutron star.
24、View larger image NASA's Chandra X-ray Observatory has discovered the first direct evidence for a superfluid, a bizarre, friction-free state of matter, at the core of a neutron star.
25、Its effect on its companion star suggested as early as 1971 that it must be a compact object with a mass too high for it to be a neutron star.
26、And whenever you make a measurement of the mass when it is a neutron star when you see the x-ray pulsations, you almost always find 4 that it is very close to 1.4 times the mass of the sun.
27、Even if you start with something (like a bump on a rotating neutron star) that gives off a perfect sine wave signal, it won't stay that way by the time it gets into the data stream.
