LOFAR radio map of the whirlpool galaxy M51 and its neighbourhood at a
frequency of 150 MHz. The field covers 4 by 2.6 degrees. The
observations were performed with the Dutch LOFAR high-band antennas. The
map shows the distribution of hot electrons in M51 and also a large
number of background galaxies.The inlay shows an enlarged view of M51 at
150 MHz (white contour lines) overlayed onto an optical image of M51
from the Digital Sky Survey (DSS). © David Mulcahy et al., Astronomy & Astrophysics
The whirlpool galaxy Messier 51 (M51) is seen from a distance of
approximately 30 million light years. This galaxy appears almost face-on and
displays a beautiful system of spiral arms.
A European team of astronomers was able to observe M51 with the International LOFAR Telescope in the frequency range 115-175 MHz, just above the normal commercial FM radio frequency band of 88-108 MHz. The team obtained the most sensitive image of any galaxy at frequencies below 1 GHz so far.
With LOFAR's high sensitivity, the disk of M51 in the radio regime could be traced much further out than before. The astronomers detected cosmic electrons and magnetic fields 40,000 light years away from the center of M51. With LOFAR's high angular resolution, the spiral arms are clearly visible. Magnetic fields and cosmic rays are densest in spiral arms. Compared to higher radio frequencies, spiral arms appear broader due to the diffusion of cosmic electrons away from the spiral arms where they have been formed.
The view of galaxies in the radio regime is different to their optical appearance.
Whereas optical images show predominantly the visible light from stars, the
radio waves unravel two constituents of galaxies that are invisible to optical
telescopes: electrons, almost as fast as light, and magnetic fields. Their role
for the stability and evolution of galaxies is increasingly under discussion.
The electrons are "cosmic ray" particles produced in the shock fronts
of giant supernova explosions. Magnetic fields are generated by dynamo
processes driven by gas motions. When the electrons spiral around the magnetic
field lines, radio waves are emitted, a process called synchrotron emission.
Its intensity increases with the number and energy of the electrons and with
magnetic field strength.
For many decades, radio astronomy has been unable to explore low
frequencies below 300 MHz because the ionosphere acts as a barrier of
low-frequency radio waves (which are completely blocked below about 10 MHz).
Sophisticated methods of data processing and superfast computers are needed to
recover the emission. Due to these technical challenges, spiral galaxies have
hardly been studied before at these very low radio frequencies. The only
observations were of poor resolution and no details could be made out.
The target of investigation in David Mulcahy's PhD project was the
beautiful spiral galaxy Messier 51 at a distance of about 30 million light
years which is visible already in a small telescope in the constellation "Canes
Venatici", not far away from the famous Big Dipper (in German: "Großer Wagen")
in the sky.
"Low-frequency radio waves are important as they carry information about
electrons of relatively low energies that are able to propagate further away
from their places of origin in the star-forming spiral arms and are able to
illuminate the magnetic fields in the outer parts of galaxies", says David
Mulcahy. "We need to know whether magnetic fields are expelled from galaxies
and what their strength is out there."
"This beautiful image, coupled with the important scientific result it
represents, illustrates the fantastic advances that can be made at low radio
frequencies with the LOFAR telescope", continues Anna Scaife from Southampton
University, co-author of the paper. "Unravelling the mysteries of magnetic
fields is crucial to understanding how our Universe works. For too long, many
of the big questions about magnetic fields have simply been untestable and this
new era of radio astronomy is very exciting."
The Low Frequency Array (LOFAR), designed and constructed by ASTRON in the
Netherlands, is a brand new radio telescope giving access to very low radio
frequencies.
© ASTRON, The Netherlands
LOFAR explores the relatively unexplored frequency range below 240 MHz and
consists of a multitude of small and simple antennas without moving parts.
LOFAR consists of 38 stations in the Netherlands, 6 stations in Germany and one
station each in the UK, France and Sweden. The novelty is the online
combination of the signals from all stations in a powerful computing cluster
located at the University of Groningen (Netherlands).
Observations of M51 with LOFAR below FM radio frequencies (at 30-80 MHz)
have already taken place. „This opens a new window to the Universe where we do
not know how galaxies will look like", concludes Rainer Beck, who supervised
David Mulcahy's PhD project. „Maybe we will see how galaxies are magnetically
connected to intergalactic space. This is a key experiment in preparation for
the planned Square Kilometre Array (SKA) that should tell us how cosmic
magnetic fields are generated."
The nature of the
low-frequency emission of M51: First observations of a nearby galaxy with LOFAR, by D.D. Mulcahy, A. Horneffer, R. Beck et al., 2014, Astronomy &
Astrophysics (DOI: 10.1051/0004-6361/201424187).
