Results 11 to 20 of about 4,621,719 (221)

Compression and ablation of the photo-irradiated molecular cloud the Orion Bar [PDF]

open access: yesNature, 2016
The Orion Bar is the archetypal edge-on molecular cloud surface illuminated by strong ultraviolet radiation from nearby massive stars. Our relative closeness to the Orion nebula (about 1,350 light years away from Earth) means that we can study the ...
J. Goicoechea   +9 more
semanticscholar   +2 more sources

[Cii] emission from L1630 in the Orion B molecular cloud. [PDF]

open access: yesAstron Astrophys, 2017
CONTEXT L1630 in the Orion B molecular cloud, which includes the iconic Horsehead Nebula, illuminated by the star system σ Ori, is an example of a photodissociation region (PDR). In PDRs, stellar radiation impinges on the surface of dense material, often
C. Pabst   +44 more
semanticscholar   +2 more sources

Isotopic evidence for primordial molecular cloud material in metal-rich carbonaceous chondrites [PDF]

open access: yesProc Natl Acad Sci U S A, 2016
Elishevah van Kooten   +9 more
semanticscholar   +2 more sources

Giant molecular cloud catalogues for PHANGS-ALMA: methods and initial results [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2021
We present improved methods for segmenting CO emission from galaxies into individual molecular clouds, providing an update to the cprops algorithms presented by Rosolowsky & Leroy.
E. Rosolowsky   +28 more
semanticscholar   +1 more source

From Diffuse Gas to Dense Molecular Cloud Cores [PDF]

open access: yes, 2020
Molecular clouds are a fundamental ingredient of galaxies: they are the channels that transform the diffuse gas into stars. The detailed process of how they do it is not completely understood. We review the current knowledge of molecular clouds and their
J. Ballesteros-Paredes   +10 more
semanticscholar   +1 more source

Turbulent molecular clouds [PDF]

open access: yesThe 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   +5 more sources

THE CALIFORNIA MOLECULAR CLOUD [PDF]

open access: yesThe 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

The Role of Magnetic Field in Molecular Cloud Formation and Evolution [PDF]

open access: yesFrontiers in Astronomy and Space Sciences, 2019
We review the role that magnetic field may have on the formation and evolution of molecular clouds. After a brief presentation and main assumptions leading to ideal MHD equations, their most important correction, namely the ion-neutral drift is described.
P. Hennebelle, S. Inutsuka
semanticscholar   +1 more source

Turbulence in Molecular Clouds [PDF]

open access: yesThe Astrophysical Journal, 1995
accepted in ApJ, compressed postscript, figures not included. Complete preprint available at http://ucowww.ucsc.edu/~dubinski/home.html or by request to dubinski@lick.ucsc ...
John Dubinski   +2 more
openaire   +4 more sources

The formation of molecular clouds [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2001
In a recent paper, Elmegreen (2000) has made a cogent case, from an observational point of view, that the lifetimes of molecular clouds are comparable to their dynamical timescales. If so, this has important implications for the mechanisms by which molecular clouds form.
S. H. Lubow   +4 more
openaire   +4 more sources

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