Tag Archive for 'X-rays'

This illustration shows the IXPE spacecraft (right) observing the blazar Markarian 501 (left). A blazar is a black hole surrounded by a disk of gas and dust with a bright jet of high-energy particles pointed toward Earth. The inset illustration shows high-energy particles in the jet (blue). When the particles hit the shock wave, depicted as a white bar, the particles become energized and emit X-rays as they accelerate. Moving away from the shock, they emit lower-energy light: first visible, then infrared, and radio waves. Farther from the shock, the magnetic field lines are more chaotic, causing more turbulence in the particle stream. Image credit: NASA / Pablo Garcia.

IXPE Spacecraft Examines Particle Acceleration in Blazar Jets

Nov 24, 2022 by News Staff

Blazars are active galactic nuclei with jets of magnetized plasma that point nearly along the line of sight. Most of the light from these extremely luminous...

An artist’s impression of a magnetar. Image credit: NASA’s Goddard Space Flight Center / S. Wiessinger.

Distant Magnetar Has Solid Surface with No Atmosphere

Nov 4, 2022 by News Staff

Magnetars are neutron stars with ultra-strong magnetic fields, which can be observed in X-rays. Polarization measurements could provide information on...

An artist’s impression of a hot Jupiter in a binary stellar system. Image credit: NASA / CXC / M. Weiss.

Hot-Jupiter Exoplanets Slow Down Aging Process for Their Host Stars

Nov 3, 2022 by News Staff

Using data from NASA’s Chandra X-ray Observatory and ESA’s XMM-Newton spacecraft, astronomers have looked for the effects of massive, close-in planets...

This composite image shows the supernova remnant Cassiopeia A, a structure resulting from the explosion of a star in the constellation of Cassiopeia. The blues represent data from NASA’s Chandra X-ray Observatory, the turquoise is from IXPE, and the gold is courtesy of the NASA/ESA Hubble Space Telescope. Image credit: NASA / CXC / SAO / NASA / MSFC / Vink et al. / STScI.

IXPE Maps Polarized X-Rays from Cassiopeia A

Oct 18, 2022 by News Staff

Cassiopeia A is a remnant that blew up as a supernova approximately 11,000 years ago. This composite image shows the supernova remnant Cassiopeia A, a...

Astronomers think GRB 221009A represents the birth of a new black hole formed within the heart of a collapsing star. In this illustration, the black hole drives powerful jets of particles traveling near the speed of light. The jets pierce through the star, emitting X-rays and gamma rays as they stream into space. Image credit: NASA / Swift / Cruz deWilde.

Astronomers Detect Record-Breaking Gamma-Ray Burst

Oct 16, 2022 by News Staff

GRB 221009A, a gamma-ray burst detected on October 9, 2022, is one of the nearest and possibly the most-energetic gamma-ray burst ever observed. It occurred...

This Chandra image shows the LTT 1445 system: LTT 1445A is the fainter source at the center of the image with the brighter resolved binary LTT 1445 BC. Image credit: NASA / Chandra / Brown et al., arXiv: 2209.11314.

Chandra Detects X-ray Emission from Exoplanet-Hosting Triple Star System

Oct 11, 2022 by Natali Anderson

The triple star system LTT 1445, at a distance of 22.5 light-years, hosts some of the nearest rocky planets. This Chandra image shows the LTT 1445 system:...

These images span a range of different types of objects, including a cluster of galaxies (SMACS J0723.3-7327), a galaxy group (Stefan’s Quintet), a star-forming nebula (Carina Nebula), and a galaxy (Cartwheel Galaxy). In each image, the X-rays from Chandra show higher-energy processes than the infrared view from Webb. Additionally, infrared data from Spitzer is included in the Stephan’s Quintet composite. Image credit: NASA / CXC / SAO / Spitzer / JPL-Caltech / Webb / ESA / CSA / STScI.

Chandra Adds X-ray Data to Webb’s Infrared Images

Oct 5, 2022 by News Staff

The Stephan’s Quintet, the Cartwheel Galaxy, the galaxy cluster SMACS J0723.3-7327, and the Carina Nebula were among the first publicly released images...

An artist’s impression of the fireball around a white dwarf. Image credit: ROSITA Collaboration / Annika Kreikenbohm.

eROSITA Detects X-rays from Nova in Fireball Phase

Sep 22, 2022 by News Staff

Novae are caused by runaway thermonuclear burning in the hydrogen-rich atmospheres of accreting white dwarfs, which leads to a rapid expansion of the atmosphere...

This composite image shows SNR 0519-69.0, a Type Ia supernova remnant in the Large Magellanic Cloud: X-ray data from Chandra with low, medium and high energies are shown in green, blue, and purple respectively, with some of these colors overlapping to appear white; optical data from Hubble shows the perimeter of the remnant in red and stars around the remnant in white. Image credit: NASA / CXC / GSFC / Williams et al. / STScI.

Astronomers Determine Age of Supernova Remnant in Large Magellanic Cloud

Sep 14, 2022 by News Staff

Light from a Type Ia supernova explosion that created the supernova remnant SNR 0519-69.0 in the Large Magellanic Cloud, a satellite galaxy of the Milky...

The main panel of this image shows a wide-field view of NGC 4424 in optical light from Hubble. The image is about 45,000 light-years wide. The inset features a close-up view of NGC 4424 that shows Chandra X-ray data (blue) plus a version of the optical data (red) that has had light from a model of NGC 4424 subtracted from the image to show other faint features. This inset image is about 1,700 light-years across. The Nikhuli star cluster is the elongated red object. Image credit: NASA / CXC / Swinburne University of Technology / Graham et al. / ESA / STScI.

Astronomers Witness ‘Black Hole Delivery System’ in Action

Aug 18, 2022 by Natali Anderson

A rare intermediate-mass black hole may have been delivered to the barred spiral galaxy NGC 4424 by another, smaller galaxy, according to an analysis of...

Zeta Ophiuchi was once in close orbit with another star, before being ejected when this companion was destroyed in a supernova explosion; infrared data from Spitzer reveal a spectacular shock wave (red and green) that was formed by matter blowing away from the star’s surface and slamming into gas in its path; data from Chandra (blue) show a bubble of X-ray emission located around the star, produced by gas that has been heated by the shock wave to tens of millions of degrees. Image credit: NASA / CXC / University of Cambridge / Sisk-Reynés et al. / NSF / NRAO / VLA / PanSTARRS.

Chandra Takes New Look at Giant Runaway Star Zeta Ophiuchi

Jul 26, 2022 by Enrico de Lazaro

Zeta Ophiuchi is a very massive, hot, bright blue star that once had a companion that exploded as a supernova. Zeta Ophiuchi was once in close orbit with...

This artist’s impression shows what the binary system VFTS 243 might look like if we were observing it up close. The system, which is located in the Tarantula Nebula in the Large Magellanic Cloud, is composed of a hot, blue star with 25 times the Sun’s mass and a black hole, which is at least nine times the mass of the Sun. The sizes of the two binary components are not to scale: in reality, the blue star is about 200,000 times larger than the black hole. Image credit: ESO / L. Calçada.

Dormant Stellar-Mass Black Hole Detected in Tarantula Nebula

Jul 18, 2022 by News Staff

The newly-detected black hole is a member of the binary system VFTS 243, which is located in the famous Tarantula Nebula in the Large Magellanic Cloud. This...

Multi-wavelength image of Westerhout 50 (red - radio, green - optical, yellow - soft X-rays, magenta - medium energy X-rays, cyan - hard X-ray emission). The eastern lobe X-ray image highlights the XMM-Newton data (with the brightening at the edge of the field of view cropped here to highlight the source emission). The western lobe X-ray image shows only partial Chandra coverage of part of the nebula. Image credit: Safi-Harb et al., arXiv: 2207.00573.

Astronomers Find Evidence for Unusual Particle Acceleration in Manatee Nebula

Jul 5, 2022 by Sergio Prostak

Using ESA’s XMM-Newton X-ray observatory, NASA’s Nuclear Spectroscopic Telescope Array (NuSTAR) and its Chandra X-ray Observatory, astronomers have...

This composite image of H1821+643 contains X-rays from Chandra (blue) that have been combined with radio data from NSF’s Karl G. Jansky Very Large Array (red) and an optical image from the PanSTARRS telescope on Hawaii (white and yellow). Image credit: NASA / CXC / University of Cambridge / Sisk-Reynés et al. / NSF / NRAO / VLA / PanSTARRS.

Chandra Finds Slow-Rotating Supermassive Black Hole in Distant Quasar

Jul 1, 2022 by News Staff

A supermassive black hole in the center of H1821+643, a quasar about 3.4 billion light-years away from Earth, is rotating at about half the speed of light. This...

In this composite image of Abell 2146, Chandra X-ray data (purple) shows hot gas, and Subaru Telescope optical data shows galaxies (red and white). Image credit: NASA / CXC / University of Nottingham / Russell et al. / NAOJ / Subaru Telescope.

Chandra Spots 1.6-Million-Light-Year-Long Shock Wave in Abell 2146

Jun 9, 2022 by News Staff

Abell 2146 is a pair of colliding galaxy clusters located approximately 2.8 billion light-years away in the constellation of Draco. In this composite image...

An artist’s impression of a black hole X-ray binary. Image credit: Instituto de Astrofísica de Canarias.

NICER Detects Echoes from Eight Black Hole X-Ray Binaries

May 2, 2022 by News Staff

As a stellar-mass black hole pulls in gas and dust from an orbiting star, it can give off spectacular bursts of X-rays that bounce and echo off the inspiraling...

The four galaxies shown in this graphic are among 29 galaxies in the sample that showed evidence for growing black holes near their centers. X-rays from Chandra (blue) have been overlaid on optical images from the NASA/ESA Hubble Space Telescope of the galaxies NGC 1385, NGC 1566, NGC 3344, and NGC 6503. The boxes that appear in the roll-over outline the location of the burgeoning black holes. Image credit: NASA / CXC / Washington State University / Baldassare et al. / ESA / STScI.

Massive Black Holes Form in Dense Stellar Environments, Study Suggests

Apr 21, 2022 by News Staff

Black holes are demolishing thousands of stars in a quest to pack on weight, according to an analysis of images of 108 galaxies taken by NASA’s Chandra...

PSR J2030+4415 generated an extremely long beam of matter and antimatter. Image credit: NASA / CXC / Stanford University / M. de Vries / NSF / AURA / Gemini Consortium.

Chandra Spots Huge Filament of Matter and Antimatter from Gamma-Ray Pulsar

Mar 15, 2022 by Enrico de Lazaro

Using NASA’s Chandra X-ray Observatory, astronomers have observed a remarkable X-ray filament generated by the gamma-ray pulsar PSR J2030+4415. PSR J2030+4415...

A visualization of the eRosita and Fermi bubbles. Image credit: ESA / Gaia / DPAC / CC BY-SA 3.0 IGO.

Giant Bubbles Above and Below Milky Way’s Center Caused by Galaxy’s Central Black Hole

Mar 11, 2022 by News Staff

In 2020, the X-ray satellite eROSITA revealed two gigantic bubbles extending to 80° above and below the center of our Milky Way Galaxy. The morphology...

X-ray spots on the surface of the magnetar SGR 1830-0645. Image credit: Younes et al., doi: 10.3847/2041-8213/ac4700.

NICER Observes Merger of X-Ray Spots on Distant Magnetar

Mar 9, 2022 by News Staff

Using NASA’s Neutron star Interior Composition Explorer (NICER), astronomers have observed the merging of multimillion-degree X-ray spots on the surface...

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