Results 1 to 10 of about 138,438 (330)
Turbulent molecular clouds [PDF]
The Astronomy and Astrophysics Review, 2012 To be published in AARv, 58 pages, 13 figures (higher resolution figures will be available on line)
Patrick Hennebelle +2 more
openaire +7 more sources
Molecular clouds in the Galaxy [PDF]
The Astrophysical Journal, 1975 The J = 1 → 0 emission of CO has been surveyed in the galactic plane between ℓ = -10° and +90° with a U beam sampling every degree. Molecular clouds emitting in the CO line are plentiful over the inner region of the Galaxy. Their greatest number occurs in the galactic nucleus and at a radius of 5.5 kpc—a distribution similar to radio H II regions and ...
N. Z. Scoville, P. M. Solomon
openalex +6 more sources
Oxygen fractionation in dense molecular clouds. [PDF]
Mon Not R Astron Soc, 2019 22 pages, 5 ...
Loison JC +15 more
europepmc +7 more sources
Molecular Clouds in Spiral Galaxies [PDF]
Symposium - International Astronomical Union, 1983 A large observational program investigating the 2.6 mm CO line in spiral galaxies is being conducted by myself and Nick Scoville using the 14 m telescope of the Five College Radio Astronomy Observatory (HPBW = 50″). Thus far we have observed 46 galaxies of types Sa, Sb, Sc and Irr, detected 31, and mapped 16.
Judith S. Young
openalex +4 more sources
The Astrophysical JournalDeep 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 +3 more sources
The Molecular Cloud Lifecycle [PDF]
Space Science Reviews, 2020 AbstractGiant molecular clouds (GMCs) and their stellar offspring are the building blocks of galaxies. The physical characteristics of GMCs and their evolution are tightly connected to galaxy evolution. The macroscopic properties of the interstellar medium propagate into the properties of GMCs condensing out of it, with correlations between e.g.
Angela Adamo +9 more
openaire +4 more sources
Magnetic field properties in star formation: A review of their analysis methods and interpretation
Frontiers in Astronomy and Space Sciences, 2022 Linearly polarized emission from dust grains and molecular spectroscopy is an effective probe of the magnetic field topology in the interstellar medium and molecular clouds.
Junhao Liu +3 more
doaj +1 more source
12CO (3–2) High-Resolution Survey (COHRS) of the Galactic Plane: Complete Data Release
The Astrophysical Journal Supplement Series, 2022 We present the full data release of the ^12 CO (3–2) High-Resolution Survey (COHRS), which has mapped the inner Galactic plane over the range of 9.°5 ≤ l ≤ 62.°3 and ∣ b ∣ ≤ 0.°5.
Geumsook Park +11 more
doaj +1 more source
A Mesofractal Model of Interstellar Cloudiness
Universe, 2022 The interstellar medium (ISM), serving as a background for the propagation of cosmic rays (CRs) and other information carriers, has a complex ragged structure.
Vladimir V. Uchaikin +1 more
doaj +1 more source
THE CALIFORNIA MOLECULAR CLOUD [PDF]
The Astrophysical Journal, 2009 Accepted for publication in the ApJ. This submission has low resolution figures. Preprint with full resolution figures can be found at http://www.cfa.harvard.edu/~clada/pubs_html/California ...
C. J. Lada, M. Lombardi, J. F. Alves
openaire +3 more sources