It is
the nearest radio galaxy.
Not exact matches
Radio telescopes have picked up intense bursts of low - frequency static from a mysterious source that may lie hidden
near the center of our Milky Way
galaxy.
Anthony Readhead of the Owens Valley
Radio Observatory at Caltech and colleagues caught two small, hot bursts traveling away from a bright
galaxy called J1415 +1320 at
near the speed of light.
Her research interests include structure, interactions, and star formation in
galaxies in the local universe and at high redshift, and she observes in optical,
near - infrared, and
radio wavelengths.
In this discovery, reported by Caltech researchers in June,
radio telescopes picked up faint traces of the organic compound propylene oxide in a vast cloud of gas and dust called Sagittarius B2, which is
near the center of our
galaxy.
The Giant Metrewave
Radio Telescope (GMRT), which is installed near Pune in India and operates in the radio band, pointed to the link between the radio emission and a galaxy by locating the origin of the elect
Radio Telescope (GMRT), which is installed
near Pune in India and operates in the
radio band, pointed to the link between the radio emission and a galaxy by locating the origin of the elect
radio band, pointed to the link between the
radio emission and a galaxy by locating the origin of the elect
radio emission and a
galaxy by locating the origin of the electrons.
They combined observations in the visible and the
near infrared from the Hubble Space Telescope with
radio observations from the Very Large Array and the Submillimeter Array to explore the effect of the turbulence, stellar radiation, and magnetic field on massive star formation in the
galaxy's nuclear ring.
The
near - to mid-IR spectral energy distribution of the
radio galaxy suggests the existence of a reddened, E (B - V) = 0.4 (+ / --RRB- 0.1 $, evolved stellar population of age > ~ 1.8 Gyr and mass 5 (+ / --RRB- 2 x 1e11 Msun.
The target object of this observation is
radio source Sagittarius B2 (Sgr B2), which is an object with strong emission, located at
near the center of our
galaxy.
Their nuclei emit jets of high - velocity gas (
near the speed of light) above and below the
galaxy — the jets interact with magnetic fields and emit
radio signals.