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Between 2000 and 2005, the name "Pulsar" has been used in Australia and New Zealand on rebadged versions of the Sylphy. This arrangement continued until the introduction of the Nissan Tiida (C11) in 2005; at this time the Pulsar name was retired. In 2013, Nissan replaced the Tiida in Australia and New Zealand with two new models badged as Pulsar.
The Crab pulsar 33-millisecond pulse period was too short to be consistent with other proposed models for pulsar emission. Moreover, the Crab pulsar is so named because it is located at the center of the Crab Nebula, consistent with the 1933 prediction of Baade and Zwicky. [ 23 ]
The digital display on received newer graphics and a Blue back light instead of the previously Orange back light. The Pulsar 150 received mechanical changes to conform to BS4 norms, leading to a loss of 1 Ps of power. The Pulsar 180 received a 230mm rear disc brake instead of a drum brake. A new model named the Pulsar NS160 was released soon after.
PSR J1614–2230 is a millisecond pulsar, a type of neutron star, that spins on its axis roughly 317 times per second, corresponding to a period of 3.15 milliseconds. Like all pulsars, it emits radiation in a beam, similar to a lighthouse . [ 4 ]
PSR J0952–0607 is a massive millisecond pulsar in a binary system, located between 3,200–5,700 light-years (970–1,740 pc) from Earth in the constellation Sextans. [6] It holds the record for being the most massive neutron star known as of 2022, with a mass 2.35 ± 0.17 times that of the Sun—potentially close to the Tolman–Oppenheimer–Volkoff mass upper limit for neutron stars.
PSR J0737−3039 is the first known double pulsar.It consists of two neutron stars emitting electromagnetic waves in the radio wavelength in a relativistic binary system.The two pulsars are known as PSR J0737−3039A and PSR J0737−3039B.
avenger cruise 220; avenger street 220; avenger street 160; freedom cng; ct100; ct110/ct110x; ct125x; pulsar rs200; pulsar n250; pulsar f250; pulsar 220f; pulsar n160
The advent of state-of-the-art digital data acquisition systems, new radio telescopes and receiver systems and the discoveries of many new pulsars advanced the sensitivity of the pulsar timing array to gravitational waves. The 2010 paper by Hobbs et al. [8] summarizes the early state of the international effort.