Parkes telescope finds new
kind of cosmic object

16 February


A team of astronomers from the UK, USA, Australia, Italy and Canada using the
CSIRO Parkes radio telescope in eastern Australia has found a new kind of cosmic
object: small, compressed 'neutron stars' that show no activity most of the
time but once in a while spit out a single burst of radio waves. The discovery
is published in this week's issue of the journal Nature [16
February 2006].

The new objects—dubbed Rotating Radio Transients or RRATs—are likely
to be related to conventional radio pulsars (small stars that emit regular pulses
of radio waves, up to hundreds of times a second). But the new objects probably
far outnumber their old cousins, the scientists say.

Eleven RRATs have been found, first detected by the Parkes Multibeam Pulsar
Survey and then observed again several times. Their isolated bursts last for
between two and 30 milliseconds. In between, for times ranging from four minutes
to three hours, they are silent.

"These things were very difficult to pin down," says CSIRO's Dr Dick
Manchester, a member of the research team and a veteran pulsar hunter. "For
each object we've been detecting radio emission for less than one second a day.
And because these are single bursts, we've had to take great care to distinguish
them from terrestrial radio interference."

By analysing the burst arrival times, the astronomers have found that 10 of
the 11 sources have underlying periods of between 0.4 seconds and seven seconds.
It is this that suggests that they are rotating neutron stars.

Because RRATs are 'silent' most of the time, the chance of being able to detect
one is low. Many more must lurk unseen in our Galaxy, the astronomers argue—perhaps
a few hundred thousand. The number of 'normal' radio pulsars in our Galaxy is
estimated to be about 100 000.

Unlike some other kinds of stars that show periodic eruptions, the RRATs show
no evidence for being in binary systems (that is, each orbiting another star).

A handful of 'normal' pulsars produce the occasional 'giant' pulse, along with
their usual train of regular, smaller pulses. The RRATs appear to differ from
these pulsars by having magnetic field strengths in the emission region about
a hundred thousand times weaker.




Dr Maura McLaughlin (Jodrell Bank Observatory, University of Manchester)

+44-(0)1477-572-672 (office)

Dr Andrew Lyne (Jodrell Bank Observatory, University of Manchester)

+44-(0)1477-572-640 (office)



Dr Dick Manchester (CSIRO Australia Telescope National Facility)

+61-(0)2-9372-4313 (office)

Dr George Hobbs (CSIRO Australia Telescope National Facility)

+61-(0)2-9372-4652 (office)



Dr Jim Cordes (Cornell University)

+1-607-255-0608 (office)

Dr Fernando Camilo (Columbia University)

+1-212-854-2540 (office)



Dr Ingrid Stairs (University of British Columbia)

+1-604-822-6796 (office)



Dr Nicolo D'Amico (University of Cagliari)

+39-070-711-80-208 (office)

+329-660-38-28 (cell)

Dr Andrea Possenti (Cagliari Astronomical Observatory)

+39-070-711-80-249 (office)



M.A. McLaughlin, A.G Lyne, D.R Lorimer, M. Kramer, A.J Faulkner, R.N Manchester,
J.M. Cordes, F. Camilo, A. Possenti, I.H. Stairs, G. Hobbs, N. D'Amico, M. Burgay
and J.T. O'Brien. "Transient radio bursts from rotating neutron stars".
439, 817-820 (16 February 2006)