Examples of using Binary pulsar in English and their translations into Greek
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It's a binary pulsar.
Tests in stronger gravitational fields are provided by the observation of binary pulsars.
Since then, several other binary pulsars have been found.
The first report of this effect was made by Taylor and co-workers at the end of 1978,four years after the discovery of the binary pulsar was reported.
Transfer of energy: the binary pulsar PSR 1913+16(1 week).
For ordinary stars like the Sun, this energy loss would be too small to be detectable, butthis energy loss was observed in 1974 in a binary pulsar called PSR1913+16.
The discovery of the binary pulsar represents an important milestone in this historical development.
However, in 1974, this energy loss was observed in a binary pulsar called PSR1913+16.
The radiation emitted by the binary pulsar is too weak to be observed on the earth with existing techniques.
The first observation of this effect is due to Hulse and Taylor,using a binary pulsar PSR1913+16 discovered in 1974.
The radiation emitted by the binary pulsar right now is too weak to be detectable on Earth with existing technology.
The first observation of a decrease in orbital period due to the emission of gravitational waves was made by Hulse and Taylor,using the binary pulsar PSR1913+16 they had discovered in 1974.
In 1974, Hulse andTaylor discovered binary pulsar PSR B1913+16, which is made up of a pulsar and black companion star.
Relativistic precession has been observed for all planets that allow for accurate precession measurements(Mercury, Venus, and Earth),as well as in binary pulsar systems, where it is larger by five orders of magnitude.
Since then, several other binary pulsars have been found, in particular the double pulsar PSR J0737-3039, in which both stars are pulsars. .
On 2 July 1974 the first signals were discovered from a binary pulsar, two neutron stars that orbit each other.
The orbiting time of the binary pulsar is less than eight hours, which can be compared with the one month our moon takes to orbit the earth.
In the early 1990s, a group of astronomersled by Donald Backer, studying what they thought was a binary pulsar, determined that a third object was needed to explain the observed Doppler shifts.
Hulse, Taylor, and other colleagues have used this first binary pulsar to make high-precision tests of general relativity, demonstrating the existence of gravitational radiation.
However, perhaps the violent perturbations of matter that take place when the two astronomical bodies in a binary star(or a binary pulsar) approach each other so closely that they fall into each other may give rise to gravitational waves that could be observed here.