The mystery of part-time pulsars

January 5, 2017 by Suraiya Farukhi
The pulsar pictured here, which resides in the Messier 82 galaxy 12 million light-years away, sends out X-ray beams that pass Earth every 1.37 seconds. Scientists studying this object with NuSTAR originally thought it was a massive black hole, but its X-ray pulse revealed its true pulsar identity. Credit: NASA/JPL-Caltech

A new discovery has upended the widely held view that all pulsars are orderly ticking clocks of the universe. A survey done at the Arecibo Observatory in Puerto Rico has fortuitously discovered two extremely strange pulsars that undergo a "cosmic vanishing act." Sometimes they are there, and then for very long periods of time, they are not.

Recognizing the existence of this strange behavior was fortuitous in itself. It took great patience on the part of a team of radio astronomers at Jodrell Bank in the UK led by Professor Andrew Lyne of the University of Manchester to confirm the existence of these mostly invisible pulsars.

Pulsars are rapidly rotating, highly magnetized neutron stars. They are about 20 miles across with masses of about 500,000 Earths. The rotation sends charged particles streaming out from the magnetic poles, causing beams of radio waves to sweep around the sky—like the light beams from a lighthouse. This results in pulses, which can be received by terrestrial radio telescopes.

Intermittent pulsars are a rarely observed population of pulsars, which have two states—one when they pulse like normal pulsars (the ON state), and another when they mysteriously fail to work, producing no radio waves at all (the OFF state). "They switch instantaneously between the states," notes Lyne. "They're ON and then they're gone, disappearing without any apparent warning."

A 34-member pulsar study team, including Dr. Andrew Seymour, a USRA postdoc at Arecibo, used the 7-beam receiver to conduct routine pulsar searches in what they call the PALFA (Pulsar Arecibo L-Band Feed Array) Survey. The two recently discovered intermittent pulsars spend most of their time in the OFF state. Three other similar pulsars are also known, but they are mostly ON.

In September 2012, one of these new objects was discovered to be emitting very bright pulses, and it was labeled PSR J1929+1357. Of 169 new pulsars, follow-up observations of half of those had been initiated at Jodrell Bank and this candidate was confirmed as a pulsar in February 2013 using the 250-ft Lovell Telescope at the second attempt. "During the next 9 months it was observed no fewer than 650 times—100 hours," said Professor Benjamin Stappers of the Jodrell Bank Center for Astrophysics and a co-author on the publication. "It was ON on only 5 occasions—just 0.8% of the time."

The most important implication of this discovery is that there must exist an extremely large number these vanishing act pulsars. The PALFA survey, which is aimed at a section of the Milky Way visible to the Arecibo dish, only covers each position in the survey once. It probably passed over 130 similar pulsars, but this was the only one that was ON at the time of observation. Furthermore, if it were not for the early signals at Jodrell Bank, this pulsar could easily have been discarded as a false detection, likely arising from radio-frequency interference. The PALFA team estimates that there are about 3,000 such intermittent pulsars in the survey area, far greater than the population of normal pulsars.

"These disappearing pulsars may far outnumber normal pulsars," said Dr. Victoria Kaspi of McGill University in Canada and the principal investigator on the PALFA project. "In fact, they may redefine what we think of as normal."

Why this odd behavior? After all, since the original pulsar discovery in 1967, they have been referred to as marvelously accurate cosmic clocks that tick steadily for millions years with a cadence that surpasses the ticking of our best laboratory clocks. But these long-term intermittent pulsars are mostly invisible, which is about as useful as having the clock on the wall that is hidden behind a curtain for most of the time.

"The explanation of the ON-OFF behavior remains a puzzle," says Seymour. "It indicates that the pulsar environment is changing, but just what those changes entail is open to debate."

Recent observations of these odd pulsars suggest that their rotational slow-down rate when OFF is only 80 percent of the rate when ON. A property of "normal" pulsars is their pulse rate slows very gradually over time. The PALFA team suspects that the stream of charged particles, which drive the radio beams emanating from the pulsar, also causes the pulsar to spin down more rapidly. When OFF, this particle stream fails for some reason and the spin down rate is reduced. But as Seymour notes, there is as yet no agreement in the pulsar community as to the ON-OFF mechanism.

The changing spin rate is inferred by calculating how many beats were missed during the pulsar's invisible phases.

PALFA surveys are ongoing, and no one can predict if and when more examples of this fascinating new phenomenon will be found. Catching another intermittent pulsar in its ON mode is up to chance. Is there another candidate out there ready to reveal its secrets, or will it forever lurk hidden in the dark unknowns of space?

Lyne hopes that follow-up measurements of PSR J1929+1357 will provide a rare insight into the physics of the emission mechanism and the changing spin-down phenomenon.

Explore further: Astronomers detect glitch in a millisecond pulsar

More information: Two long-term intermittent pulsars discovered in the PALFA Survey. arxiv.org/abs/1608.09008

Related Stories

Astronomers detect glitch in a millisecond pulsar

June 17, 2016

(Phys.org)—European astronomers have uncovered evidence of a small glitch in the spin of a millisecond pulsar. According to a research paper published on June 13 on arXiv.org, the pulsar, designated PSR J0613-0200, exhibits ...

Pulsar wind nebulae

November 7, 2016

Neutron stars are the detritus of supernova explosions, with masses between one and several suns and diameters only tens of kilometers across. A pulsar is a spinning neutron star with a strong magnetic field; charged particles ...

Millisecond pulsars

October 3, 2016

When a star with a mass of roughly ten solar masses finishes its life, it explodes as a supernova, leaving behind a neutron star as remnant "ash." Neutron stars have masses of one-to-several suns but they are tiny in diameter, ...

Discovery of the companions of millisecond pulsars

September 28, 2015

When a star with a mass of roughly ten solar masses finishes its life, it does so in a spectacular explosion known as a supernova, leaving behind as remnant "ash" a neutron star. Neutron stars have masses of one-to-several ...

Astronomers find six new millisecond pulsars

January 26, 2016

(Phys.org)—NASA's Fermi Gamma-ray Space Telescope has once again proven that it is an excellent tool to search for rotating neutron stars emitting beams of electromagnetic radiation, known as pulsars. A team of astronomers, ...

Recommended for you

Uncovering the origins of galaxies' halos

November 21, 2017

Using the Subaru Telescope atop Maunakea, researchers have identified 11 dwarf galaxies and two star-containing halos in the outer region of a large spiral galaxy 25 million light-years away from Earth. The findings, published ...

Recurring martian streaks: flowing sand, not water?

November 20, 2017

Dark features on Mars previously considered evidence for subsurface flowing of water are interpreted by new research as granular flows, where grains of sand and dust slip downhill to make dark streaks, rather than the ground ...

2 comments

Adjust slider to filter visible comments by rank

Display comments: newest first

Chris_Reeve
1 / 5 (5) Jan 05, 2017
Re: "'The explanation of the ON-OFF behavior remains a puzzle,' says Seymour. 'It indicates that the pulsar environment is changing, but just what those changes entail is open to debate.'"

It's an anomaly for their spinning lighthouse model, but as the researchers note, not so much for any explanation of pulsars which positions the pulses as a function of the environment.

Add this to the other anomaly that these things are observed to "spin" at the rate of a dentist's drill, and you've now got two separate anomalies which both point to a more electrical explanation.

Let's not forget that a relaxation oscillator is a sophomore-level EE project which can replicate the basic features of this pulsating class of objects without any need to propose hypothetical neutronium when the "spin rates" get too high.
Tuxford
1 / 5 (5) Jan 05, 2017
they have been referred to as marvelously accurate cosmic clocks that tick steadily for millions years with a cadence that surpasses the ticking of our best laboratory clocks.

The aliens simply have more accurate clocks. They turn on and off their galactic GPS beacons, powered by stars, at their convenience, perhaps only when navigating in certain regions.

Please sign in to add a comment. Registration is free, and takes less than a minute. Read more

Click here to reset your password.
Sign in to get notified via email when new comments are made.