magnetar tagged posts

World’s first 3D Simulations of Superluminous Supernovae


The nebula phase of the magnetar-powered super-luminous supernova from our 3D simulation. At the moment, the supernova ejecta has expanded to a size similar to the solar system. Large scale mixing appears at the outer and inner region of ejecta. The resulting light curves and spectra are sensitive to the mixing that depends on stellar structure and the physical properties of magnetar. Credit: Ken Chen

For most of the 20th century, astronomers have scoured the skies for supernovae—the explosive deaths of massive stars—and their remnants in search of clues about the progenitor, the mechanisms that caused it to explode, and the heavy elements created in the process. In fact, these events create most of the cosmic elements that go on to form new stars, galaxies, and life.

Because no...

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Simulations Reveal the Invisible Chaos of Superluminous Supernovae

1. Astrophysicist Ken Chen ran 2D simulations with Berkeley Lab's CASTRO code on NERSC's Edison supercomputer to better understand the physical conditions that create superluminious supernova. Credit: Ken Chen, National Astronomical Observatory of Japan 2. Superluminous Supernova simulation in 2D generated with Berkeley Lab developed CASTRO code. (Credit: Ken Chen, National Astronomical Observatory of Japan)

1. Astrophysicist Ken Chen ran 2D simulations with Berkeley Lab’s CASTRO code on NERSC’s Edison supercomputer to better understand the physical conditions that create superluminious supernova.
Credit: Ken Chen, National Astronomical Observatory of Japan 2. Superluminous Supernova simulation in 2D generated with Berkeley Lab developed CASTRO code. (Credit: Ken Chen, National Astronomical Observatory of Japan)

Sightings of a rare breed of superluminous supernovae – stellar explosions that shine 10 to 100 times brighter than normal – are perplexing astronomers. First spotted only in last decade, scientists are confounded by the extraordinary brightness of these events and their explosion mechanisms...

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Young Magnetar Likely the Slowest Pulsar Ever Detected

Supernova Remnant RCW 103

This composite image shows RCW 103 and its central source, known officially as 1E 161348-5055 (1E 1613, for short), in three bands of X-ray light detected by Chandra. In this image, the lowest energy X-rays from Chandra are red, the medium band is green, and the highest energy X-rays are blue. The bright blue X-ray source in the middle of RCW 103 is 1E 1613. The X-ray data have been combined with an optical image from the Digitized Sky Survey.

Using NASA’s Chandra X-ray Observatory and other X-ray observatories, astronomers have found evidence for what is likely one of the most extreme pulsars, or rotating neutron stars, ever detected...

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Astronomers find the first ‘Wind Nebula’ around a Magnetar

This artist's rendering shows a magnetar outburst. A 2011 outburst of Swift J1834.9-0846 led to its discovery by NASA's Swift satellite. Credit: NASA's Goddard Space Flight Center

This artist’s rendering shows a magnetar outburst. A 2011 outburst of Swift J1834.9-0846 led to its discovery by NASA’s Swift satellite. Credit: NASA’s Goddard Space Flight Center

Astronomers have discovered a vast cloud of high-energy particles called a wind nebula around a rare ultra-magnetic neutron star, or magnetar, for the first time. The find offers a unique window into the properties, environment and outburst history of magnetars, which are the strongest magnets in the universe.

A neutron star is the crushed core of a massive star that ran out of fuel, collapsed under its own weight, and exploded as a supernova. Each one compresses the equivalent mass of half a million Earths into a ball just 12 miles across, or about the length of New York’s Manhattan Island...

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