Not exact matches
However, recent high - resolution
radio images of some winged
galaxies show sharp breaks where a pair
of jets angles off in a new direction, rather than sweeping out gradual curves.
Santiago Garcia - Burillo
of Spain's Madrid Observatory and his colleagues have used a
radio telescope array in Chile to
image the torus
of NGC 1068, a
galaxy 50 million light years away.
Images of four distant
galaxies observed with the Arecibo
radio telescope, which have been found to host huge reservoirs
of atomic hydrogen gas.
Looking at a distant
galaxy: the
radio chart (left) shows the
image of the blazar PKS 1830 - 211 distorted by the gravitational lens effect.
Gas surrounds a giant black hole in the early universe in this
radio image, but astronomers see little evidence for a massive
galaxy of stars.
Radio / Optical combination
images of distant
galaxies as seen with NSF's Very Large Array and NASA's Hubble Space Telescope.
Like any spiral
galaxy, M106 has a pair
of arms full
of bright young stars (green), but researchers have long wondered at the source
of its two extra arms (purple and blue), visible in
radio and X-ray
images.
Using the combined power
of nine
radio telescopes arrayed across the Southern Hemisphere, the
images reveal features just 15 light - days across in the heart
of the nearby
galaxy Centaurus A, 12 million light - years away.
ALMA is a telescope suitable for analyzing molecules in
galaxies because
of: 1) a high sensitivity to detect faint
radio signals; 2) a high fidelity imaging capability to
image actual gas distributions; 3) the ability to observe wideband multiple wavelengths simultaneously, and high spatial resolution.
The astronomers began their quest by using the VLBA to make very high resolution
images of more than 1,200
galaxies, previously identified by large - scale sky surveys done with infrared and
radio telescopes.
Using the millimeter - wave interferometer at Caltech's Owens Valley
Radio Observatory, the astronomers combined 15 smaller
images into a single mosaic to produce an
image showing the location
of Carbon Monoxide (CO) gas throughout a
galaxy called IC 10, some 2.5 million light - years away.
The spiral
galaxy M51: Left, as seen with the Hubble Space Telescope; Right,
radio image showing location
of Carbon Monoxide gas.
The scientists used the National Science Foundation's Very Large Array (VLA)
radio telescope in New Mexico and the Westerbork Synthesis Radio Telescope (WSRT) in the Netherlands to produce an image of the galaxy M33, known to amateur astronomers as the Pinwheel Ga
radio telescope in New Mexico and the Westerbork Synthesis
Radio Telescope (WSRT) in the Netherlands to produce an image of the galaxy M33, known to amateur astronomers as the Pinwheel Ga
Radio Telescope (WSRT) in the Netherlands to produce an
image of the
galaxy M33, known to amateur astronomers as the Pinwheel
Galaxy.
The large - scale optical and
radio structures previously have been thought to indicate the symmetry axis
of the active nucleus in the inner light - months
of the
galaxy, an idea now called into question by the new VLBA
images.
Figure 1 Composite
image showing how powerful
radio jets from the supermassive black hole at the center
of a
galaxy in the Phoenix Cluster inflated huge «bubbles» in the hot, ionized gas surrounding the
galaxy (the cavities inside the blue region
imaged by NASA's Chandra X-ray observatory).
VLBA false - color representation
of the
radio image of the center
of the Seyfert
galaxy NGC 4151, 43 million light years from Earth.
VLBA false - color representation
of the
radio image of the center
of the Seyfert
galaxy NGC 4151, made at a wavelength
of 18 cm.
The
radio structure at the center
of the Seyfert
galaxy NGC 4151, located approximately 43 million light - years from Earth, was
imaged with a resolution
of better than 1 light - year.
Drs. Alan Roy and James Ulvestad
of the National
Radio Astronomy Observatory, together with Drs. Edward Colbert and Andrew Wilson of the Space Telescope Science Institute and the University of Maryland, used the VLBA to image a light - year - sized radio jet in NGC 4151, a relatively nearby spiral ga
Radio Astronomy Observatory, together with Drs. Edward Colbert and Andrew Wilson
of the Space Telescope Science Institute and the University
of Maryland, used the VLBA to
image a light - year - sized
radio jet in NGC 4151, a relatively nearby spiral ga
radio jet in NGC 4151, a relatively nearby spiral
galaxy.
«This shows how well such
radio images of the gas distribution in
galaxies can reveal evidence
of galactic interactions,» Lim said.
A combined optical -
radio image of the quasar IRAS 17596 +4221 and a companion
galaxy.
When the first space - based
radio telescope, HALCA, launched from Japan in 1997, our VLA and VLBA paired with it to take
images of galaxies at a level
of detail never before achieved.
Now an international team
of researchers from eight different countries has made ultra-high angular resolution
images of the black hole jet at the centre
of the giant
galaxy NGC 1275, also known as
radio source Perseus A or 3C 84.
IMAGE: Artistic composition
of the
radio telescopes in space and on the ground observing NGC 1275, the central
galaxy of the Perseus cluster
of galaxies at a distance
of 230 million... view more
New
radio images of galaxies with bright quasar cores show that, though the
galaxies appear normal in visible - light
images, their gas has been disrupted by encounters with other
galaxies.
«The polarization
of the waves coming from the background quasar, combined with the fact that the waves producing the two lensed
images traveled through different parts
of the intervening
galaxy, allowed us to learn some important facts about the
galaxy's magnetic field,» said Sui Ann Mao, Minerva Research Group Leader for the Max Planck Institute for
Radio Astronomy in Bonn, Germany.
With the combined power
of a worldwide network
of radio telescopes, astronomers hope to peer into the heart
of our
galaxy and
image — for the first time — the very edges
of a black hole.