Astronomers are interested in binary pulsars because they provide unique laboratories for testing theories of gravity and fundamental physics. These systems allow researchers to study the effects of strong gravitational fields and the impact of relativistic effects, such as gravitational wave emission. Additionally, binary pulsars can help in measuring the masses of neutron stars and contribute to our understanding of stellar evolution. Their precise timing also aids in probing the behavior of matter under extreme conditions.
Mainly astronomers. But cosmologists and astrophysicists will also be interested in outer space.
Pulsars have extremely short periods; in some cases seconds, in some cases just a few milliseconds. There is no way a typical star, with its great size (for example, a diameter of 1.4 million kilometers in the case of our Sun) can pulsate that quickly.
B
The Pulsars was created in 1994.
Nekkar is a binary star system located in the constellation of Cygnus. It consists of two stars, with the primary star being a red giant and the secondary a main-sequence star. Nekkar is notable for its brightness and is often studied in the context of stellar evolution and interactions in binary systems. Its precise characteristics make it an interesting subject for astronomers interested in stellar dynamics.
Pulsars are studied by astronomers.
Because I am interested in neutron stars.
Pulsars are detected by their regular pulses of radiation - hence the name. If I remember correctly, that is radio waves. Before the nature of pulsars was known, the first pulsars discovered were named LGM-1, LGM-2, LGM-3, and LGM-4 - where LGM is short for "little green men". An astronomers' joke.
Cepheid Variables.
Mainly astronomers. But cosmologists and astrophysicists will also be interested in outer space.
The most likely navigation system that we might use after leaving the Solar System would be a system using rapidly spinning pulsars as navigational beacons. Each pulsar spins with a distinctive period; by seeing three or more pulsars and measuring the bearings to each, we can figure out where we are in space. In fact, when astronomers first discovered pulsars, they dubbed them "LGM signals", for "little green men"; the pulses were SO regular that they couldn't be natural, astronomers thought. Therefore, these must actually BE interstellar navigational beacons! Now, of course, astronomers have figured out what they are, and no longer believe them to be artificial. But pulsars still might be interstellar navigational beacons even if they ARE natural.
Pulsars have extremely short periods; in some cases seconds, in some cases just a few milliseconds. There is no way a typical star, with its great size (for example, a diameter of 1.4 million kilometers in the case of our Sun) can pulsate that quickly.
B
The Pulsars ended in 2000.
The Pulsars was created in 1994.
Astronomers first assumed that the millisecond pulsar was very young because its high speed of rotation suggested that it had undergone a significant amount of spin-up in a short period of time. This led them to believe that it had been spun-up recently, which is typically associated with young pulsars.
Nekkar is a binary star system located in the constellation of Cygnus. It consists of two stars, with the primary star being a red giant and the secondary a main-sequence star. Nekkar is notable for its brightness and is often studied in the context of stellar evolution and interactions in binary systems. Its precise characteristics make it an interesting subject for astronomers interested in stellar dynamics.