Most radio galaxies are elliptical galaxies.
Not exact matches
As the
most abundant element in the Universe and the raw fuel for creating stars, hydrogen is used by
radio astronomers to detect and understand the makeup of other
galaxies.
Most SETI researchers look for signals sent by sentient beings in
radio waves, because these waves traverse
galaxies without interference from gas and dust.
Among the
most exotic beasts in the astrophysical zoo are millisecond pulsars, which spin hundreds of times every second while flashing
radio beams across the
galaxy.
The
most distant
radio - quiet
galaxy previously known has a red shift of 2.758.
Clues to what our
Galaxy, the Milky Way, was like in its infancy may come from a newly discovered «normal» (
radio - quiet)
galaxy, the
most distant of its kind ever seen.
For this reason the
most readily detectable
radio signals from another civilization may come from outside our
galaxy.
By 2000
radio astronomers had found almost all of them in various dust clouds throughout our
galaxy, suggesting that the interplay between ice and gas may be one of the
most important mechanisms for synthesizing the precursors of life.
The
most fascinating feature of this
galaxy is its jet, which is visible in optical light as well as x-rays and
radio emissions.
This FRB, which lasted for only a few thousandths of a second, was unique, as it contained invaluable information about the cosmic web — the swirling, diffuse and faint web of gases and magnetic fields that exists between
galaxies, and which is completely invisible to optical and
most radio telescopes.
Although it is close to the line of sight to the globular cluster M15,
most astronomers had thought that this source of bright
radio waves was probably a distant
galaxy.
This portion of the spectrum, which is more energetic than
most radio waves yet less energetic than visible and infrared light, holds the key to understanding a great variety of fundamental processes, including planet and star formation, and the formation and evolution of
galaxies and
galaxy clusters in the early Universe.
Scientists believe that understanding the origin and nature of FRBs could even provide invaluable information about the cosmic web — the swirling, diffuse and faint web of gases and magnetic fields that exists between
galaxies, and which is completely invisible to optical and
most radio telescopes.