Astronomers found a low-mass companion to a rapidly spinning pulsar, which orbits the neutron star every 54.7 minutes at an average distance of 230,000 miles. The system is thought to have formed billions of years ago and is now accreting mass from the companion, causing an outburst.
Researchers using Arecibo Telescope discovered never-before-seen radio emission spectra from the Crab Nebula pulsar. The findings suggest an unknown magnetic pole, contradicting existing theories and challenging our understanding of pulsars.
Astronomers have used a pair of pulsars to show that general relativity is correct within 0.05% accuracy, the most stringent limit to date. The double-pulsar system provides independent tests of general relativity and its predictions, including gravitational waves and time dilation.
A US-Australian research team has detected radio pulses from a magnetar star, XTE J1810-197, which is giving off extraordinary radio pulses. The finding links this rare type of star with the much more common 'radio pulsars', reordering our understanding of these neutron stars.
Astronomers have discovered a unique pulsar that is only 'on' for part of the time, shedding light on how pulsars emit regular beams of radio waves. The pulsar, PSR B1931+24, slows down 50% faster when it's active compared to when it's not.
Researchers precisely measured the mass of a millisecond pulsar, PSR J1909-3744, using precise pulse arrival time measurements and disentangled the Shapiro delay effect from Roemer delay. The result reveals the white dwarf companion's mass to be 1.44 times that of the sun with an uncertainty of 0.02 solar masses.
The PULSE collaboration has achieved outstanding scientific results by studying pulsars to test fundamental laws and understand extreme conditions. They discovered the first known double pulsar, confirming Einstein's general theory of relativity.
A total of eight new VHE gamma-ray sources have been found in the Milky Way's disc, doubling known sources at these energies. The discovery includes two 'dark accelerators' without obvious counterparts in other wavelength bands, sparking excitement among astronomers.
Astronomers have discovered the smallest extra-solar planet to date, orbiting a pulsar in a planetary system resembling our own inner solar system. The new planet is estimated to be one-fifth the mass of Pluto and has an orbit approximately six times larger than its third planet.
Professor Jim Hough of the University of Glasgow believes that gravitational waves will be detected in the near future due to advancements in instrument technology. The UK's GEO 600 device has shown promising results, and its innovations are being considered by LIGO for implementation.
Gravitational waves are ripples in space-time produced by massive objects' acceleration. The detection of these waves will provide unique information about astrophysical systems like supernovae and black hole formation.
A UBC-led research team has confirmed the existence of the universe's oldest and farthest planet, a gas giant formed 13 billion years ago. The ancient world takes a century to complete each orbit and is unlikely to support life due to its metal-poor composition.
The XMM-Newton satellite has discovered a faint X-ray glow from a very hot gas in the disk of the Andromeda Galaxy, suggesting recent star formation. Additionally, the team detected an accreting X-ray pulsar, a strongly magnetized neutron star drawing in material from its neighbor.
Researchers discovered pulsar bursts coming from beachball-sized structures in the Crab Nebula, a cloud of debris from a supernova. The structure's small size is inconsistent with all but one proposed theory for generating radio emission.
Researchers are using computer simulations to determine if the 47 Ursae Majoris system can contain an Earth-like planet. The system's asteroid belt is in the habitable zone, increasing the likelihood of finding a terrestrial planet.
Researchers using NASA's Chandra X-ray Observatory have discovered a probable pulsar at the center of a 1,600-year-old supernova. The finding provides evidence for an associated pulsar and allows for detailed study of the supernova remnant. This discovery helps connect pulsars with massive stars from which they formed.
A team of astronomers has confirmed a key aspect of Einstein's general theory of relativity by measuring the precise orbit of a pulsar. The study used sophisticated instruments to record over 50,000 Gigabytes of data and demonstrated the predicted delay in radio pulses traveling through curved space-time.
Scientists confirm pulsar formed in 386 AD supernova, a historic event witnessed by Chinese astronomers. The discovery, using NASA's Chandra X-ray Observatory, provides strong evidence for the pulsar's age and sheds new light on the behavior of young neutron stars.
Researchers using Chandra X-ray Observatory associate a pulsar with a historic supernova, dated back to 386 AD, providing strong evidence for the young age of the pulsar. The discovery challenges conventional wisdom on pulsars and their formation.
Chandra has revealed unprecedented images of a blast wave from an exploding star, a flare from a brown dwarf, and a small galaxy being cannibalized by a larger one. The observatory's high resolution has enabled scientists to pinpoint sources of the X-ray background glow, leading to a better understanding of our universe.
Researchers using the VLA radio telescope found a pulsar that is at least 40,000 years old and may be as old as 170,000 years. This discovery challenges current understanding of neutron stars and their ages.
Researchers propose two theories to explain the origin of neutron star kicks: the 'mass rocket,' which suggests a mass ejection asymmetry, and the 'neutrino rocket,' which relies on the intense magnetic field surrounding the newly formed neutron star. These theories aim to explain the observed high speeds of pulsars and the asymmetrica...
New Chandra X-ray Observatory images reveal a luminous spike from a giant black hole, a compact nebular resembling a cosmic crossbow, and a hot bubble of gas surrounding a dying star. These observations contradict theoretical predictions, indicating the presence of high-energy particles beyond expectations.
Researchers have observed an 'earthquake' in a slow-spinning, highly magnetic collapsed star, confirming it as a neutron star. The finding supports the magnetar hypothesis and provides strong evidence for the existence of these rare objects.
The 'braking glitch' in the spin rate of a soft gamma repeater (SGR) suggests a massive starquake may have occurred. The SGR's rotational period increased steadily until a rapid decrease was observed, indicating a massive energy release.
Researchers have produced a new radio image revealing a supernova remnant and numerous pulsar candidates, showcasing the Milky Way's central region in unprecedented detail. The technique will be useful for astronomers to study the galaxy's major components.
Astronomers have discovered a large number of slow X-ray pulsars in supernova remnants, which are believed to be neutron stars with huge magnetic fields. These so-called magnetars rotate much slower than expected and are invisible to radio probes.
A new pulsar has been discovered orbiting a massive star, providing insights into the mysterious behavior of transient objects. The pulsar, named XTE J1946+274 or GRO J1944+26, exhibits complex orbital patterns and intense magnetic fields, challenging our understanding of these enigmatic celestial bodies.
A rapidly spinning neutron star can naturally produce a Gamma-ray burst by oscillating and radiating its rotation energy. The spin-down process is triggered by the gravitational wave instability, which grows explosively in hours or minutes, strengthening the magnetic field and eventually radiating away all remaining rotation energy.
Astronomers Renyue Cen suggests that gamma-ray bursts might come from supernovae expelling material at high speeds, producing jets that travel at nearly the speed of light. This theory could explain why some pulsars are moving faster than ordinary stars and potentially pose a catastrophic threat to Earth.
A rapidly spinning neutron star, SAX J1808.4-3658, is providing proof for the theory that millisecond pulsars are propelled to mind-boggling speeds by accretion of material from a companion star. This discovery fills an important niche in our understanding of star evolution.
Cornell University astronomers James Cordes and Barney Rickett have developed a method to calculate the speed and distance of extremely fast-moving neutron stars, called pulsars, by analyzing their twinkling rate. By combining data from two large radio telescopes, they can identify new pulsars and better understand their physics.
A NASA scientist has found a new puzzle in the sky, an X-ray pulsar that appears to burst twice every 'year' rather than once. Colleen Wilson discovered GRO J2058+42, which has no visible component and exhibits unusual behavior, suggesting it may be a binary star system with a type Be star and a neutron star in a lopsided orbit.
Researchers found that accreting pulsars exhibit strange behavior, including gaining and losing time, due to mass transfer from stellar companions. This phenomenon is caused by the negative torque experienced by the pulsar, which affects its spin rate.
A team of scientists discovered that the Pioneer 10 spacecraft detected a radio signal modulation mimicking a planet's orbit around PSR B1257+12. The analysis reveals that solar rotation causes similar variations in the pulsar's radio waves, effectively simulating the planet.