Results 31 to 40 of about 4,653,928 (371)

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

12 CO, 13CO, AND C18 OBSERVATIONS TOWARD OMC-1 [PDF]

open access: yesJournal of Astronomy and Space Sciences, 2002
Interstellar cabon monoxide and its isotopes were observed with the 13.7m radio telescope of the Daeduk Radio Astronomy Observatory toward Orion Molecular Cloud-1 (OMC-1).
Mun-Suk Chun   +2 more
doaj   +1 more source

Anatomy of Orion Molecular Clouds—The Astrochemistry Perspective/Approach

open access: yesFrontiers in Astronomy and Space Sciences, 2021
The Orion molecular cloud (OMC) complex is the nearest and perhaps the best-studied giant molecular cloud complex within which low-mass and massive star formation occur. A variety of molecular species, from diatomic molecules to complex organic molecules
Dipen Sahu, Sheng-Yuan Liu, Tie Liu
doaj   +1 more source

A Velocity Structure Analysis of Giant Molecular Cloud Associated with HII Region S152 [PDF]

open access: yesJournal of Astronomy and Space Sciences, 2005
S152 is a small bright emission nebula located in the Perseus arm. Its optical diameter corresponds to 1.5 pc for an adopted distance 3.5 kpc. However, S152 is a part of a giant molecular cloud complex, which consists of several dense cores, containing ...
Woo-Yeol Choi   +3 more
doaj   +1 more source

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

A novel in-situ method to determine the respiratory tract deposition of carbonaceous particles reveals dangers of public commuting in highly polluted megacity

open access: yesParticle and Fibre Toxicology, 2022
Background Exposure to air pollutants is one of the major environmental health risks faced by populations globally. Information about inhaled particle deposition dose is crucial in establishing the dose–response function for assessing health-related ...
Leizel Madueño   +5 more
doaj   +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 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

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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