Not exact matches
Astronomers used a radio telescope
called the Atacama Large Millimeter /
submillimeter Array (ALMA) to look for organic molecules in the Large Magellanic Cloud, located about 160,000 light - years from Earth.
Now, researchers have used a galaxy simulation
called FIRE (Feedback In Realistic Environments), developed at Northwestern University, Evanston, in Illinois, to model a
submillimeter galaxy with as fine a resolution as they could achieve.
Remy Indebetouw, an astronomer at the University of Virginia in Charlottesville, and colleagues took another stab using a new high - resolution telescope network
called the Atacama Large Millimeter /
submillimeter Array (ALMA) in Chile.
Therefore, the research group targeted molecular line emissions from hydrogen cyanide (HCN), formyl ion (HCO +), and hydrogen sulfide (CS) at millimeter /
submillimeter wavelengths (* 4) in the galaxy
called NGC 1097 (about 50 million light years away) with the ALMA Telescope in the Atacama Desert in Chile.
A research group led by Anne Dutrey from the Laboratory of Astrophysics of Bordeaux, France and CNRS used the Atacama Large Millimeter /
submillimeter Array (ALMA) to observe the distribution of dust and gas in a multiple - star system
called GG Tau - A [1].
Combining the capabilities of two powerful telescopes, the Atacama Large Millimeter /
submillimeter Array (ALMA) and Hubble Space Telescope, astronomers have explored the nature of a mysterious huge object
called «Himiko» in the early universe.
ALMA observations cover a range of wavelengths
called «millimeter /
submillimeter» waves.