Not exact matches
Looking back on the failed
radio observations at the turn
of the millennium, Disney is eager to make up for lost time and continue the search for the phantom universe's elusive
galaxies.
«When more - powerful detectors provide us with more
observations,» Mészáros said, «we also will be able to use Fast
Radio Bursts as a probe
of their host
galaxies,
of the space between
galaxies,
of the cosmic - web structure
of the universe, and as a test
of fundamental physics.»
Those
observations, published today in Nature, reveal that the location
of the bursts coincides with a faint, remote
galaxy that also hosts a faint, persistent source
of radio waves.
This plot shows
observations of the
galaxy from the Owens Valley
Radio Observatory in California (black), the Metsähovi
Radio Observatory in Finland (blue) and the Submillimeter Array in Hawaii (red).
Observations of two
galaxies made with the National Science Foundation - funded Atacama Large Millimeter / submillimeter Array (ALMA)
radio telescope suggest that large
galaxies formed faster than scientists had previously thought.
Observations of the shock between this pair
of clusters showed that the
radio emission was connected to the
galaxy's jet, so clearly the electrons must have been initially accelerated by the black hole and then reaccelerated by the shock waves.
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.
Those
observations reveal that the location
of the bursts coincides with a faint, remote
galaxy that also hosts a persistent source
of radio waves.
Science Interests Formation
of galaxies and black holes in the early universe and their growth over cosmic time; large surveys with Hubble and other telescopes to discover new populations
of distant
galaxies and black holes; physical properties
of active galactic nuclei using
observations from
radio, infrared, optical, ultraviolet through to X-ray energies.
NICMOS
observations of high redshift
radio galaxies: witnessing the formation
of bright elliptical
galaxies?
Since the research team had already conducted
radio observations of various molecular emissions in this galaxy with the 45 - m telescope at the Nobeyama Radio Observatory of NAOJ, they aimed to develop their research further with ALMA and identify the difference in chemical composition between AGNs and starburst reg
radio observations of various molecular emissions in this
galaxy with the 45 - m telescope at the Nobeyama
Radio Observatory of NAOJ, they aimed to develop their research further with ALMA and identify the difference in chemical composition between AGNs and starburst reg
Radio Observatory
of NAOJ, they aimed to develop their research further with ALMA and identify the difference in chemical composition between AGNs and starburst regions.
Instead, we found this black hole fleeing from the larger
galaxy and leaving a trail
of debris behind it,» U.S. National
Radio Astronomy Observatory's James Condon — the lead author
of a study detailing the
observations — said in a statement released Wednesday.
UT1 is determined from measurements
of the rotation
of the Earth by various means including
radio telescope
observations of quasars (distant
galaxies powered by supermassive black holes).
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.
The GBT has joined Spektr - R in several
observations of active galactic nuclei, the supermassive black holes lurking inside
galaxies that are bright in
radio waves.
Dr. Lockman's area
of research is the structure and evolution
of the Milky Way and nearby
galaxies, with a special emphasis on
radio observations of neutral...
The main science targets specific to these Hubble
observations are the host
galaxies of Green Double
Radio - lobed Active Galactic Nuclei (Green DRAGN — pronounced Green Dragon) and Spiral Double
Radio - lobed Active Galactic Nuclei (S - DRAGN).
Observations with
radio and infra - red telescopes show that NGC 5128 swallowed a spiral
galaxy probably about five hundred million years ago and the effects
of the collision powers the strong
radio emission.
Her research is focused on using
radio observations of novae and symbiotic systems to examine the evolution
of accreting dwarf
galaxies among other things.
Nodland and Ralston said that their analysis
of previous
radio observations of 160
galaxies, made in the 1970s and 1980s, showed that radiation coming from objects had its direction
of polarization rotated by different amounts, depending on the direction
of the
galaxies.
Abstract: A follow - up X-ray study was made
of the west lobe
of the
radio galaxy Fornax A, (NGC 1316) based on new ASCA
observations made in 1997 for 98 ks, and incorporating the previous
observation in 1994 for 39 ks.
Astronomer Vera Cooper Rubin found over decades
of radio observations that the rotational velocity
of clouds
of ionized hydrogen (HII regions) in spiral
galaxies like the Milky Way was not decreasing at increasing distance from their galactic cores, like the velocity
of the planets around the Sun.