Institute of Astronomy

Astronomers discover the ‘Mighty Mouse’ of stellar remnants

Published on 08/10/2014 

An international team of astronomers has found a pulsating, dead star beaming with the energy of about 10 million suns. This is the brightest pulsar – a dense stellar remnant left over from a supernova explosion – ever recorded.

“You might think of this pulsar as the ‘Mighty Mouse’ of stellar remnants,” said Fiona Harrison of the California Institute of Technology. “It has all the power of a black hole but with much less mass.”

The discovery, made with NASA's Nuclear Spectroscopic Telescope Array (NuSTAR), is helping astronomers better understand mysterious sources of fierce X-rays, called ultraluminous X-ray sources, or ULXs. Before now, all ULXs were thought to be black holes. New data from NuSTAR show that at least one ULX, about 12 million light-years away in the galaxy Messier 82 (M82), is actually a pulsar.

“The pulsar appears to be eating the equivalent of a black hole diet,” said Harrison, NuSTAR principal investigator.

The discovery, reported in the October 9 issue of the journal Nature, will help astronomers understand how black holes gorge, and grow, so quickly – an important event in the formation of galaxies and structures in the universe.

“This is a surprising and fascinating discovery,” said Professor Andy Fabian of Cambridge’s Institute of Astronomy, one of the paper’s co-authors. “The true nature of ULXs has remained hidden since their discovery about 20 years ago and now one of them is shown to be a pulsar which is nearly 100 times brighter than it should be, according to current accretion ideas. We're all wondering how many other ULXs are similar.”

ULXs are generally thought to be black holes feeding, or accreting, off companion stars. They are suspected to be the long-sought medium-size black holes – missing links between smaller, stellar-size black holes and the gargantuan ones that dominate the hearts of all galaxies. But research into the true nature of ULXs is ongoing.

NuSTAR didn't initially set out to study the two ULXs in M82. Astronomers had been observing a recent supernova in M82, when they noticed a pulse of bright X-rays coming from a point nearby – what turned out to be the ULX called M82 X-2. Black holes don't pulse, but pulsars do.

Pulsars belong to a class of stars called neutron stars. Like black holes, neutron stars are the burnt-out cores of exploded stars, only puny in mass by comparison. Pulsars, discovered by Cambridge’s Jocelyn Bell and Antony Hewish in 1967, are neutron stars that send out beams of light. As the star spins, these beams intercept Earth like lighthouse beacons, producing a pulsed signal.

“We took it for granted that the powerful ULXs must be massive black holes,” said Matteo Bachetti, lead author of the paper from the University of Toulouse. “When we first saw the pulsations in the data, we thought they must be from another source.”

NASA's Chandra X-ray Observatory and Swift satellite had also been monitoring M82 to study the same supernova, and confirm that the intense X-rays of M82 X-2 were coming from a pulsar.

“Having a diverse array of telescopes in space means that they can help each other out,” said Paul Hertz, director of NASA's astrophysics division in Washington. “When one telescope makes a discovery, others can be called in for backup.”

The key to NuSTAR's discovery was in its sensitivity to X-rays in the highest-energy ranges as well as its ability to precisely measure the timing of the signals. This timing capability allowed the astronomers to measure a pulse rate from M82 X-2 of 1.37 seconds. They also measured its energy output at the equivalent of 10 million suns, or 10 times more than what was measured before – a big punch for something about the mass of the sun and half the size of Cambridge.

How is this puny dead star radiating so fervently? Astronomers aren't sure, but they say it is likely due to a lavish feast of the cosmic kind. As is the case with black holes, the gravity of a neutron star can pull matter off companion stars. As the matter is dragged into the neutron star, it heats up and glows with X-rays. If the pulsar is indeed feeding off surrounding matter, it is doing so at such an extreme rate to have theorists scratching their heads.

Astronomers are planning follow-up observations with NuSTAR, Swift and Chandra to help explain the bizarre behavior. The NuSTAR team will also look at more ULXs, and it's possible they could turn up more pulsars. At this point, it is not clear if the M82 X-2 is an oddball or if more ULXs beat with the pulse of dead stars. NuSTAR, a relatively small telescope, has thrown a big loop into the mystery of black holes.

IoA Contact: Prof AC Fabian, Institute of Astronomy, University of Cambridge

acf@ast.cam.ac.uk

Link to the Nature paper

   

 

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Page last updated: 8 October 2014 at 19:02