Astronomers studying a black hole in our Galaxy with ESA’s XMM-Newton
observatory have made a surprising discovery about the cocktail of
particles that are ejected from its surroundings.
Stellar-mass black holes are often found feasting on material from a
companion star. Matter flows from the star towards the black hole,
circling in a disc around it with a temperature so high that it emits
X-rays.
The black hole can be a fussy eater: instead of swallowing all of the
material, it sometimes pushes a fraction of it away in the form of two
powerful jets of particles. Because these jets release mass and energy
into the surroundings, the black hole has less material to feed on.
By studying the composition of the jets, we can learn more about the feeding habits of black holes.
Observations at radio wavelengths have already found that black hole
jets contain electrons moving at close to the speed of light. But, until
now, it was not clear whether the negative charge of the electrons is
complemented by their anti-particles, positrons, or rather by heavier
positively-charged particles in the jets, like protons or atomic nuclei.
In a new study, astronomers have used XMM-Newton to study a black hole
binary system called 4U1630–47, well known to show outbursts of X-rays
over periods of months and years.
“In our observations, we found signs of highly ionised nuclei of two
heavy elements, iron and nickel,” says María Díaz Trigo of the European
Southern Observatory in Munich, Germany, lead author of the paper
published in the journal Nature.
“The discovery came as a surprise – and a good one, since it shows
beyond doubt that the composition of black hole jets is much richer than
just electrons.”
The team of astronomers observed 4U1630–47 with XMM-Newton on two
occasions in September 2012, and compared the results with
near-simultaneous radio observations from the Australia Telescope
Compact Array.
Although the two sets of observations described by Dr Díaz Trigo and
collaborators were separated by only a couple of weeks, the results were
surprisingly different.
In the first set of observations, the astronomers detected X-rays from
the accretion disc, but did not see anything in radio waves – a sign
that the jets were not active.
But in the second set, they detected the source both in X-rays and radio
waves, so they knew the jets had been reactivated in the meantime.
When scrutinising the X-ray data from the second batch of observations,
the astronomers also found tell-tale signs of iron nuclei moving both
towards and away from XMM-Newton, providing confirmation that the ions
belong to the two jets, pointing in opposite directions.
The astronomers also found evidence of nickel nuclei in the jet pointing towards XMM-Newton.
“From these ‘fingerprints’ of iron and nickel, we could show that the
speed of the jet is very high, about two-thirds of the speed of light,”
says co-author James Miller-Jones from the Curtin University node of the
International Centre for Radio Astronomy Research in Perth, Australia.
“Moreover, the presence of heavy atomic nuclei in black hole jets means
that mass and energy are being carried away from the black hole in much
larger amounts than we previously thought, which may have an impact on
the mechanism and rate by which the black hole accretes matter,” adds
co-author Simone Migliari from the University of Barcelona, Spain.
This is the first time that heavy nuclei have been detected in the jets of a relatively typical stellar-mass black hole.
There is only one other X-ray binary that shows similar signatures from
atomic nuclei in its jets – a source known as SS 433. This black hole
system, however, is characterised by an unusually high accretion rate,
which makes it difficult to compare its properties to those of more
ordinary black holes.
The new observations of 4U1630–47 will help astronomers learn more about
the physical mechanism that launches jets from a black hole’s accretion
disc.
“While we now know a great deal about black holes and what happens
around them, the formation of jets is still a big puzzle, so this
observation is a major step forward in understanding this fascinating
phenomenon,” says Norbert Schartel, ESA's XMM-Newton Project Scientist.
“Baryons in the relativistic jets of the stellar-mass black hole candidate 4U1630–47,” by M. Díaz Trigo et al. is published in Nature, 14 November 2013.
For further information, please contact:
Markus Bauer
ESA Science and Robotic Exploration Communication Officer
Tel: +31 71 565 6799
Mob: +31 61 594 3 954
Email: markus.bauer@esa.int
María Díaz Trigo
European Southern Observatory, Munich, Germany
Email: mdiaztri@eso.org
Norbert Schartel
XMM-Newton Project Scientist
Tel: +34 91 8131 184
Email: Norbert.Schartel@sciops.esa.int
Source: ESA
