Results 71 to 80 of about 14,604 (166)

Molecular Clouds Resolved at the Onset of Cosmic Noon

open access: yesThe Astrophysical Journal Letters
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

open access: yesFrontiers in Astronomy and Space Sciences, 2020
Derek Ward-Thompson   +3 more
doaj   +1 more source

3D MC. I. X-Ray Tomography Begins to Unravel the 3D Structure of a Molecular Cloud in our Galaxy’s Center

open access: yesThe Astrophysical Journal Letters
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

open access: yesThe Astrophysical Journal
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
doaj   +1 more source

Oxygen fractionation in dense molecular clouds. [PDF]

open access: yesMon Not R Astron Soc, 2019
Loison JC   +15 more
europepmc   +1 more source

The Molecular Clouds of M31

open access: yesThe Astrophysical Journal
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

3D CMZ. III. Constraining the 3D Structure of the Central Molecular Zone via Molecular Line Emission and Absorption

open access: yesThe Astrophysical Journal
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]

open access: yesNature, 2019
Kruijssen JMD   +9 more
europepmc   +1 more source

Erratum: Submillimeter and Far-Infrared Polarimetric Observations of Magnetic Fields in Star-Forming Regions

open access: yesFrontiers in Astronomy and Space Sciences, 2019
Frontiers Production Office
doaj   +1 more source

Home - About - Disclaimer - Privacy