Tag Archive for 'Pulsar'

A thermonuclear blast on a pulsar called SAX J1808.4-3658 resulted in the brightest burst of X-rays seen to date by NASA’s Neutron star Interior Composition Explorer. Image credit: NASA’s Goddard Space Flight Center.

NICER Detects Thermonuclear Burst from X-Ray Pulsar

Nov 8, 2019 by News Staff

NASA’s Neutron star Interior Composition Explorer (NICER) has detected an extremely energetic explosion called a Type I X-ray burst from SAX J1808.4-3658,...

Astronomers Find Most Massive Neutron Star Ever Discovered

Sep 17, 2019 by News Staff

Astronomers using NSF’s Green Bank Telescope have identified a record breaking neutron star with the highest mass yet known. The object, called MSP J0740+6620,...

Glitch in Vela Pulsar Provides Unique Opportunity to Study Neutron Star’s Interior

Aug 13, 2019 by News Staff

Pulsars are rapidly rotating neutron stars observed to have pulses of radiation at very regular intervals that typically range from milliseconds to seconds....

Macleod et al analyzed the properties of vacuum Cherenkov radiation in strong laser pulses and the magnetic field around a pulsar. Image credit: Gerd Altmann.

High-Velocity Charged Particles Emit Cherenkov Radiation in Quantum Vacuum

May 6, 2019 by News Staff

According to new research published in the journal Physical Review Letters, charged particles traveling through empty space can emit Cherenkov radiation...

The CTB 1 supernova remnant resembles a ghostly bubble in this image, which combines new 1.5 GHz observations from the Very Large Array (orange, near center) with older observations from the Dominion Radio Astrophysical Observatory’s Canadian Galactic Plane Survey (1.42 GHz, magenta and yellow; 408 GHz, green) along with infrared data (blue). The VLA data clearly reveal the straight, glowing trail from PSR J0002+6216 and the curved rim of the remnant’s shell. Image credit: Jayanne English, University of Manitoba / NRAO / F. Schinzel et al / DRAO / Canadian Galactic Plane Survey / NASA / IRAS.

Astronomers Find Pulsar Hurtling Through Space

Mar 22, 2019 by News Staff

Astronomers using NASA’s Fermi Gamma-ray Space Telescope and NSF’s Karl G. Jansky Very Large Array have spotted a pulsar hurtling through space at...

In this composite image of Kes 75, high-energy X-rays observed by Chandra are colored blue and highlight the pulsar wind nebula surrounding the pulsar, while lower-energy X-rays appear purple and show the debris from the explosion. Image credit: X-rays – NASA / CXC / NCSU / S. Reynolds; optical – PanSTARRS.

Milky Way’s Youngest Pulsar Confirmed

Oct 23, 2018 by News Staff

Astronomers using NASA’s Chandra X-ray Observatory have confirmed that a supernova remnant called Kes 75 contains the youngest known pulsar in our Milky...

An artist’s impression of the strong magnetic neutron star Swift J0243.6+6124 launching a jet. Image credit: ICRAR / University of Amsterdam.

Highly Magnetic Neutron Star Unexpectedly Shoots Jet of Material

Sep 28, 2018 by News Staff

Astronomers using NSF’s Karl G. Jansky Very Large Array have discovered a fast-moving jet of material propelled outward from a strongly magnetized neutron...

This image shows RX J0806.4-4123 with a disk of warm dust that produces an infrared signature as detected by the NASA/ESA Hubble Space Telescope. Image credit: NASA / ESA / Nahks Tr’Ehnl, Pennsylvania State University.

Hubble Detects Unusual Infrared Emission from Nearby Neutron Star

Sep 18, 2018 by News Staff

An unusual infrared emission from the neutron star RX J0806.4-4123 detected by the NASA/ESA Hubble Space Telescope could indicate new features never before...

Unlike most supernovae that fade away, SN 2012au continues to shine today thanks to a powerful new pulsar. Image credit: NASA / ESA / J. DePasquale, STScI.

Astronomers Witness Birth of Pulsar from Energetic Supernova Explosion

Sep 14, 2018 by News Staff

A team of astronomers has observed a new phenomenon in the aftermath of SN 2012au, an extremely energetic supernova discovered on March 14, 2012 in the...

An artist’s impression of the triple star system PSR J0337+1715, which is located about 4,200 light-years from Earth. Image credit: NRAO / AUI / NSF / S. Dagnello.

Scientists Test Einstein’s Theory of Gravity on Unique Triple-Star System

Jul 5, 2018 by News Staff

In a new test of Einstein’s theory of gravity, a group of astronomers from the Netherlands, the United States, Australia and Canada has demonstrated...

PSR B1957+20 is seen in the background through the cloud of gas enveloping its brown dwarf companion. Image credit: Mark A. Garlick / Dunlap Institute for Astronomy & Astrophysics, University of Toronto.

Plasma Lenses Amplify Pulsar Emission in Rare Binary System

May 24, 2018 by Enrico de Lazaro

A group of astronomers at the University of Toronto in Canada has performed one of the highest resolution observations in the history of astronomy by observing...

This artist’s impression depicts IGR J17062–6143. Image credit: NASA’s Goddard Space Flight Center.

NASA’s Neutron Star Interior Composition Explorer Finds Pulsar in Ultracompact Orbit

May 11, 2018 by News Staff

Astronomers using NASA’s Neutron star Interior Composition Explorer (NICER) have found evidence that an accreting millisecond X-ray pulsar called IGR...

This illustration shows NASA’s NICER mission at work aboard the International Space Station. Image credit: NASA’s Goddard Space Flight Center.

NASA Engineers Demonstrate Pulsar-Based Navigation in Space

Jan 16, 2018 by News Staff

NASA engineers have successfully demonstrated X-ray navigation in space — a capability that could revolutionize NASA’s ability in the future to...

The globally distributed dishes of the European VLBI Network are linked with each other and the 305-m William E. Gordon Telescope at the Arecibo Observatory in Puerto Rico. Together they have localized FRB121102’s exact position within its host galaxy. Image credit: Danielle Futselaar, www.artsource.nl.

Fast Radio Burst Source Linked to Extreme Magnetic Environment

Jan 11, 2018 by News Staff

Using the Arecibo Observatory in Puerto Rico and the Green Bank Telescope in West Virginia, astronomers have gained new insight into the extreme home of...

HAWC map for the region around Geminga (about 815 light-years away in the constellation Gemini) and PSR B0656+14 (about 940 light-years away). Image credit: John Pretz.

Nearby Pulsars Shed Light on Origin of Excess Antimatter

Nov 17, 2017 by News Staff

Astrophysicists using the High-Altitude Water Cherenkov (HAWC) Gamma-Ray Observatory in Mexico have detected the extended emission of high-energy gamma...

Composite image of the X-ray pulsar SXP 1062 surrounded by the supernova remnant. The false-color image combines X-ray (blue) and optical data (oxygen - green, hydrogen - red). Image credit: ESA / XMM-Newton / L. Oskinova, University of Potsdam / M. Guerrero, Instituto de Astrofisica de Andalucia / Cerro Tololo Inter-American Observatory / R. Gruendl & Y. H. Chu, University of Illinois at Urbana-Champaign.

Astronomers Observe ‘Glitch’ in Binary Pulsar for First Time

Sep 8, 2017 by News Staff

The discovery of the largest timing irregularity yet observed in a pulsar is the first confirmation that binary pulsars (pulsars orbiting with a companion...

PSR J0952-0607 (lower right) rotates 707 times a second and now ranks as second-fastest pulsar known. The location of LOFAR’s first millisecond pulsar discovery, PSR J1552+5437, which spins 412 times a second, is shown at upper left. Image credit: NASA / DOE / Fermi LAT Collaboration / ASTRON.

Second-Fastest-Spinning Pulsar Found

Sep 6, 2017 by News Staff

An international team of astronomers has discovered a pulsar — the core of a massive star that exploded as a supernova — spinning at more than...

Swift J0042.6+4112 is brighter at high energies than the Andromeda galaxy’s entire black hole population. The inset image shows the pulsar candidate in blue, as seen in X-ray light by NASA’s NuSTAR mission. The background image of the Andromeda galaxy was taken by NASA’s Galaxy Evolution Explorer in UV light. Image credit: NASA / JPL-Caltech / GSFC / JHU.

Astronomers Solve Mystery of Andromeda’s Hard X-Rays

Mar 28, 2017 by News Staff

The Andromeda galaxy (also known as Messier 31) features a dominant source of hard X-rays, but its identity was mysterious until now. An international...

NGC 5907 X-1 is in the spiral galaxy NGC 5907, which is also known as the Knife Edge Galaxy or Splinter Galaxy. This image comprises X-ray emission data (blue/white) from ESA’s XMM-Newton space telescope and NASA’s Chandra X-ray observatory, and optical data from the Sloan Digital Sky Survey. The inset shows the X-ray pulsation of the spinning neutron star, which has a period of 1.13 sec, as determined by XMM-Newton’s European Photon Imaging Camera. Image credit: ESA / XMM-Newton / NASA / Chandra / SDSS.

XMM-Newton Spots Record-Breaking Pulsar: NGC 5907 X-1

Feb 24, 2017 by News Staff

ESA’s XMM-Newton mission has spotted a pulsar — a rapidly rotating, magnetized neutron star that sweeps regular pulses of radiation in two symmetrical...

This artist’s impression shows AR Scorpii. In this unique double star a rapidly spinning white dwarf star (right) powers electrons up to almost the speed of light. These high energy particles release blasts of radiation that lash the companion red dwarf star (left) and cause the entire system to pulse dramatically every 1.97 minutes with radiation ranging from the ultraviolet to radio. Image credit: M. Garlick / University of Warwick / ESO.

Astronomers Find First Ever White Dwarf Pulsar

Feb 13, 2017 by News Staff

Astronomers have identified AR Scorpii — a binary stellar system in the constellation Scorpius, 380 light-years from Earth — as the first example...

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