Results 71 to 80 of about 14,604 (166)
Molecular Clouds Resolved at the Onset of Cosmic Noon
We present the discovery of seven molecular clouds in the radio galaxy B2 0902+34 at redshift z = 3.4. These clouds are detected as CO(0–1) absorption features against the bright radio continuum and spectrally resolved using the Karl G. Jansky Very Large
Bjorn H. C. Emonts +12 more
doaj +1 more source
Editorial: The Role of Magnetic Fields in the Formation of Stars
Derek Ward-Thompson +3 more
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Astronomers have used observations of the Galactic gas and dust via infrared, microwave, and radio to study molecular clouds in extreme environments such as the Galactic center.
Samantha W. Brunker +7 more
doaj +1 more source
Velocity Structure and Molecular Formation in the Polaris Molecular Cloud
We present a wide-field $(60^{\prime} \times 30^{\prime} )$ study of a dense region within the Polaris Flare using ^12 CO, ^13 CO, and C ^18 O ( J = 1–0) observations at 15″ resolution, obtained with the Nobeyama 45 m Radio Telescope.
Tomomi Shimoikura +3 more
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Oxygen fractionation in dense molecular clouds. [PDF]
Loison JC +15 more
europepmc +1 more source
Deep interferometric observations of CO and dust continuum emission are obtained with the Submillimeter Array at 230 GHz to investigate the physical nature of the giant molecular cloud (GMC) population in the Andromeda galaxy (M31).
Charles J. Lada +3 more
doaj +1 more source
Effects of grain alignment efficiency on synthetic dust polarization observations of molecular clouds. [PDF]
King PK, Chen CY, Fissel LM, Li ZY.
europepmc +1 more source
The Milky Way’s Central Molecular Zone (CMZ) is the largest concentration of dense molecular gas in the Galaxy, the structure of which is shaped by the complex interplay between Galactic-scale dynamics and extreme physical conditions.
Daniel L. Walker +17 more
doaj +1 more source
Fast and inefficient star formation due to short-lived molecular clouds and rapid feedback. [PDF]
Kruijssen JMD +9 more
europepmc +1 more source

