Results 11 to 20 of about 3,546,850 (294)

HCO+ in dark molecular clouds [PDF]

open access: yesSerbian Astronomical Journal, 2007
Formyl ion is one of the most important molecules, and primary molecular ion to be found in molecular clouds. This paper reviews chemical pathways of formation and destruction of the molecule, as well as its use as a tool in the study of dark molecular ...
Nikolić S.
doaj   +2 more sources

The Correlation Between Dust and Gas Contents in Molecular Clouds

open access: yesThe Astronomical Journal
Molecular clouds are regions of dense gas and dust in space where new stars and planets are born. There is a strong correlation between the distribution of dust and molecular gas in molecular clouds.
Rui-Zhi Li   +5 more
doaj   +2 more sources

The Molecular Cloud Lifecycle [PDF]

open access: yesSpace 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.
Chevance, Mélanie   +8 more
openaire   +3 more sources

Submillimetre molecular line observations and modelling of molecular clouds. [PDF]

open access: yes, 1985
PhDSubmillimetre molecular line observations of molecular clouds in our galaxy are presented, and the data analysed using various alternative cloud models.
Richardson, Kevin John
core   +4 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   +2 more sources

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 ...
Dubinski, John   +2 more
openaire   +2 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.
Pringle, J. E.   +2 more
openaire   +2 more sources

Fragmentation in molecular clouds [PDF]

open access: yesSymposium - International Astronomical Union, 1991
B209. Fragments are detected in the outer parts of the B209 molecular cloud in a region of density 1000 cm −3 using 12 CO, 13 CO, H 2 CO, IRAS 60 and 100
Frank O. Clark   +2 more
openaire   +1 more source

Molecular line signatures of cloud–cloud collisions [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2021
ABSTRACT Collisions between interstellar gas clouds are potentially an important mechanism for triggering star formation. This is because they are able to rapidly generate large masses of dense gas. Observationally, cloud collisions are often identified in position–velocity (PV) space through bridging features between intensity peaks ...
Priestley, F. D., Whitworth, A. P.
openaire   +3 more sources

Thermal desorption of water ice in the interstellar medium [PDF]

open access: yes, 2001
Water (H2O) ice is an important solid constituent of many astrophysical environments. To comprehend the role of such ices in the chemistry and evolution of dense molecular clouds and comets, it is necessary to understand the freeze-out, potential surface
Collings, Mark P.   +10 more
core   +4 more sources

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