pulsar

There may be a real physical cause for dispersion of the pulsars out of the plane.

Only a tiny fraction of pulsars is in binary systems where their masses can be determined.

To see two pulsars orbiting each other in a binary system is extremely rare in itself.

The uniqueness of this class of objects and certain shared features argue in fact that all pulsars have such an origin.

Searches for binary radio pulsars so far were called "acceleration searches" or "sideband searches" .

Pulsars and Supernovae are shown on the sky because scientists believe they emit gravitational waves.

Pulsars are the dense cores left over after stars of a certain mass explode into supernovae.

Unlike past uses of pulsars to probe gravitational waves, this technique picks up the direct effects of the waves.

Pulsars can emit gravitational waves by a variety of mechanisms in the sensitive frequency range of ground-based detectors.

Pulsars are widely thought to be rapidly rotating, magnetized neutron stars.

Will it detect new pulsars, black holes, or perhaps some novel natural phenomenon of which we have no inkling?

Pulsars and supernovas seem to take over at about 9: 00 and are truly spectacular.

Astronomers keep discovering new noisemakers in space: colliding black holes, glitching pulsars, gamma ray bursts.

When pulsars, as they became named, were discovered in the 1960s, they were nicknamed LGM for "little green men. "

Pulsars are rotating neutron stars that are observable as sources of electromagnetic radiation.

However, we should be aware that pulsars may not be neutron stars at all, they may be Strange Stars!

Radio pulsars are neutron stars with an immensely strong magnetic field.

The purple dots represent the known pulsars , which have been detected electromagnetically.

This procedure doesn't work as well for pulsars in most short-period binary systems.

Interest was renewed in the astronomical community with the discovery of pulsars .

A decade ago, he says, very little was known about any connections between pulsars and magnetars.

Some neutron stars become pulsars , stars that send off pulses of radio waves. These can also cause gravitational waves.

The limited sensitivity of present pulsar surveys and the greater frequency drift make the more distant pulsars difficult to observe.

In addition to extraterrestrial signals we might see signs of evaporating black holes or discover new pulsars.

Thus, a significant fraction of pulsars are being missed in the surveys.

This is when I concentrated on pulsars and built a large machine to do realtime processing of pulsar radio signals, right at the telescope.

Pulsars: Neutron Stars or Strange Stars?

From this, most young radio pulsars are inferred to have magnetic fields between 1012 and 1013 gauss.

The solution emerged from an entirely separate line of work, on radio pulsars .

XMM-Newton discovered X-ray emission from both pulsars in October 2006.

These are pulsars -- the dense, fast-spinning, and intensely magnetic leftovers of exploded stars.

For example, spinning neutron stars called pulsars emit clocklike streams of electromagnetic pulses.

speeding up in the rotational periods of binary stars and pulsars

Turbulence, Dynamos, Accretion Disks, Pulsars and Collective Plasma Processes ( Astrophysics and Space Science Proceedings )

Positioning for a Spacecraft using Pulsars

Research Progress and developments Prospectsof millisecond pulsars timing method

Research on the Spacecraft Autonomous Navigation Using Pulsars

Progress in the Studies of Interstellar Scintillation of Pulsars

A Three-dimensional Outer-magnetospheric Gap Model for Crab-like Pulsars

Research on Analysis and Processing Methods for Weak Signal and Noise of Pulsars

The Critical Rotation of Strange Stars and Rapidly Rotating Pulsars

Evidence of Deconfinement of Quark Matters in the Observation of Pulsars

The expected high energy radiation from anomalous X-ray pulsars

The high-energy emission from millisecond pulsars

Bulk Viscosity of QM and Limiting Rotation for Pulsars

A research on the timing method and the development of millisecond pulsars