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The Crab Pulsar (PSR B0531+21 or Baade's Star) is a relatively young neutron star. The star is the central star in the Crab Nebula, a remnant of the supernova...

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...

The Crab Nebula (catalogue designations M1, NGC 1952, Taurus A) is a supernova remnant and pulsar wind nebula in the constellation of Taurus. The common...

supernova remnant, for example the Crab Nebula, or the nebula within the large Vela Supernova Remnant. As the pulsar wind nebula ages, the supernova remnant...

An optical pulsar is a pulsar which can be detected in the visible spectrum. There are very few of these known: the Crab Pulsar was detected by stroboscopic...

constellation Crab Nebula, the supernova remnant found in the constellation Taurus Crab Pulsar, the central star in the Crab Nebula Crab (unit), photometrical...

TeV has been detected from the Vela pulsar and together with the Crab pulsar at 1.5 TeV are the only two known pulsar with emission in this energy range...

{\displaystyle P\!\approx 33} ms of the Crab pulsar using Arecibo Observatory. After this discovery, scientists concluded that pulsars were rotating neutron stars...

Cosmic Cannonball Radio pulsar Recycled pulsar PSR B1937+21 Low mass X-ray pulsar (LMXP) Accretion-powered pulsar Anomalous X-ray pulsar (AXP) AXP 1E 1048-59...

Crab Pulsar. The observation, which verified the POLIX instrument's operation, took place between January 15 and 18, 2024. POLIX monitored the Crab Pulsar...

Crab Pulsar lies at the centre of the nebula. The Moche people of ancient Peru worshipped nature, especially the sea, and often depicted crabs in their...

discovered the optical component of the Crab Pulsar in 1969 with John Cocke, which was the first optical pulsar ever observed. He was one of the pioneers...

the Crab Nebula. It is located in the sky near the star Zeta Tauri (ζ Tauri). The core of the exploding star formed a pulsar, called the Crab Pulsar (or...

synchrotron emission is important is pulsar wind nebulae, also known as plerions, of which the Crab nebula and its associated pulsar are archetypal. Pulsed emission...

instability structure is evident in the Crab Nebula, in which the expanding pulsar wind nebula powered by the Crab pulsar is sweeping up ejected material from...

Gaensler, B. M.; Anderson, J. (2008). "A Precise Proper Motion for the Crab Pulsar, and the Difficulty of Testing Spin-Kick Alignment for Young Neutron...

discovery of pulsars in 1967, optical images of the Crab Nebula taken by Keeler in 1899 were used to determine the proper motion of the Crab Pulsar. Keeler...

the first neutron star was not observed until 1967 when the first radio pulsar was discovered, neutron stars were proposed by Baade and Zwicky in 1933...

Indian astronomers measuring the variations of X-ray polarisation of the Crab Pulsar in the Taurus constellation. This study was a project conducted by scientists...

In studies of the Vela and Crab pulsars, jets have been observed which are believed to align with the spin axis of the pulsar. Since these jets align very...