MAGNATAR
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MAGNATAR
Magnatar Drop Weighty First Single from ‘Crushed’
~Doomed & Stoned Debuts~
By Billy Goate
Artwork by Sienna Langone
There's some study floating around on the internets that has concluded most people solidify their musical interests -- including a set number of bands -- by the mid-20s. From personal experience, I can say this is largely true. I will always be drawn to my staple of Alice in Chains, Soundgarden, and Nine Inch Nails. Yet I've never truly stopped searching for new sounds that speak to me. This requires a willingness to wade through the morass of releases bombarding the heavy music community on the daily. Often it takes 100 albums before I find a band that's doing something different or at least filling out a tried and true form with heart and soul.
New Hampshire four-piece MAGNATAR struck me immediately as a band that's striving to see what's just beyond view of the naked eye. Their sound is continually pushing forward with bold sweeping gestures. One could almost characterize it as monstrous, but truthfully it is both beast and beauty. There are moments on 'Crushed' (2022) when the vents are opened up and all hell is cast through them. Other songs on the album usher us through valleys of wonder ("Crown of Thorns"), mountains of disturbing mystery ("Crushed"), and apocalyptic landscapes dotted with meteoric craters ("Even Horizon").
Today, Doomed & Stoned is hosting the world premiere of the first single from this 8-track epic. "Dragged Across the Surface of the Sun" is like a grand announcement: we’re now approaching the sun; prepare for the dragging. The jutting rhythmic structure meted out by John Funk (drums) and Andrews Pagliuca (bass) reminds me of Meshuggah, with their machine-like precision. But this is doomed sludge, so the unhurried tempo really allows us to soak in those massive reverberating chords and revel in the fuming tremolos that greet us two minutes in.
Eric Sauter's vocals are mean 'n' dirty (he also produced the record, giving ample space for atmosphere). Inching closer towards a chorus, his roars are contrasted with secondary vocals that are clean, soaring, and emotive. The combined tone of Eric Sauter and Colin Ward's guitars conjure Monolord levels of heaviness that'll please a big slice of this readership.
Says the band:
The whole album is about a long relationship I was in that turned physically abusive from their side. It's a trip through the slow burn of having one's dignity broken down piece by piece, feeling trapped and unable to escape the life you're living in as you mistake abuse as love. It also highlights watching someone you love succumb to addiction and lose complete control of themselves, seeing the darkest most evil parts of humans through those combined experiences.
"Dragged" is a journey through the state of being emotionally and physically abused, the inability to see the harm being caused to you while you try to find the love in it
We can anticipate Magnatar's debut LP Crushed to drop on June 3rd c/o Seeing Red Records. I'm envisioning this on a playlist with Yob, Neurosis, Helms Alee, Ken Mode, Torche, King Bastard, and Terminus.
Give ear...
Crushed by Magnatar
SOME BUZZ
Since 2017, Magnatar have commanded their presence through high voltage amplified atmosphere. Assembled in the mountainous state of New Hampshire, the quad brings about a sound rife with hellish, off-metered dissonance and drone, introspective ambient passages, and a vocal style that transitions between harsh and hypnotic. After an EP release in 2017 & an extended single release in 2018, their debut album, 'Crushed' (2022), is by far their most concentrated and fierce release to date.
Photography by Mike Villars
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https://scitechdaily.com/our-galaxys-brightest-gamma-ray-binary-system-may-be-powered-by-a-magnetar-star/
A team of researchers led by members of the Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU) has analyzed previo
Finally getting around to properly designing a magnatar god for MPYF. X_X
Astronomers find the first 'wind nebula' around a magnetar 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 (20 kilometers) across, or about the length of New York's Manhattan Island. Neutron stars are most commonly found as pulsars, which produce radio, visible light, X-rays and gamma rays at various locations in their surrounding magnetic fields. When a pulsar spins these regions in our direction, astronomers detect pulses of emission, hence the name. Typical pulsar magnetic fields can be 100 billion to 10 trillion times stronger than Earth's. Magnetar fields reach strengths a thousand times stronger still, and scientists don't know the details of how they are created. Of about 2,600 neutron stars known, to date only 29 are classified as magnetars. The newfound nebula surrounds a magnetar known as Swift J1834.9-0846 -- J1834.9 for short -- which was discovered by NASA's Swift satellite on Aug. 7, 2011, during a brief X-ray outburst. Astronomers suspect the object is associated with the W41 supernova remnant, located about 13,000 light-years away in the constellation Scutum toward the central part of our galaxy. "Right now, we don't know how J1834.9 developed and continues to maintain a wind nebula, which until now was a structure only seen around young pulsars," said lead researcher George Younes, a postdoctoral researcher at George Washington University in Washington. "If the process here is similar, then about 10 percent of the magnetar's rotational energy loss is powering the nebula's glow, which would be the highest efficiency ever measured in such a system." A month after the Swift discovery, a team led by Younes took another look at J1834.9 using the European Space Agency's (ESA) XMM-Newton X-ray observatory, which revealed an unusual lopsided glow about 15 light-years across centered on the magnetar. New XMM-Newton observations in March and October 2014, coupled with archival data from XMM-Newton and Swift, confirm this extended glow as the first wind nebula ever identified around a magnetar. A paper describing the analysis will be published by The Astrophysical Journal. "For me the most interesting question is, why is this the only magnetar with a nebula? Once we know the answer, we might be able to understand what makes a magnetar and what makes an ordinary pulsar," said co-author Chryssa Kouveliotou, a professor in the Department of Physics at George Washington University's Columbian College of Arts and Sciences. The most famous wind nebula, powered by a pulsar less than a thousand years old, lies at the heart of the Crab Nebula supernova remnant in the constellation Taurus. Young pulsars like this one rotate rapidly, often dozens of times a second. The pulsar's fast rotation and strong magnetic field work together to accelerate electrons and other particles to very high energies. This creates an outflow astronomers call a pulsar wind that serves as the source of particles making up in a wind nebula. "Making a wind nebula requires large particle fluxes, as well as some way to bottle up the outflow so it doesn't just stream into space," said co-author Alice Harding, an astrophysicist at NASA's Goddard Space Flight Center in Greenbelt, Maryland. "We think the expanding shell of the supernova remnant serves as the bottle, confining the outflow for a few thousand years. When the shell has expanded enough, it becomes too weak to hold back the particles, which then leak out and the nebula fades away." This naturally explains why wind nebulae are not found among older pulsars, even those driving strong outflows. A pulsar taps into its rotational energy to produce light and accelerate its pulsar wind. By contrast, a magnetar outburst is powered by energy stored in the super-strong magnetic field. When the field suddenly reconfigures to a lower-energy state, this energy is suddenly released in an outburst of X-rays and gamma rays. So while magnetars may not produce the steady breeze of a typical pulsar wind, during outbursts they are capable of generating brief gales of accelerated particles. "The nebula around J1834.9 stores the magnetar's energetic outflows over its whole active history, starting many thousands of years ago," said team member Jonathan Granot, an associate professor in the Department of Natural Sciences at the Open University in Ra'anana, Israel. "It represents a unique opportunity to study the magnetar's historical activity, opening a whole new playground for theorists like me." ESA's XMM-Newton satellite was launched on Dec. 10, 1999, from Kourou, French Guiana, and continues to make observations. NASA funded elements of the XMM-Newton instrument package and provides the NASA Guest Observer Facility at Goddard, which supports use of the observatory by U.S. astronomers. TOP IMAGE....This X-ray image shows extended emission around a source known as Swift J1834.9-0846, a rare ultra-magnetic neutron star called a magnetar. The glow arises from a cloud of fast-moving particles produced by the neutron star and corralled around it. Color indicates X-ray energies, with 2,000-3,000 electron volts (eV) in red, 3,000-4,500 eV in green, and 5,000 to 10,000 eV in blue. The image combines observations by the European Space Agency's XMM-Newton spacecraft taken on March 16 and Oct. 16, 2014. Credit ESA/XMM-Newton/Younes et al. 2016 LOWER IMAGE....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