Results 101 to 110 of about 219,513 (216)
Internal 1000 au Scale Structures of the R CrA Cluster-forming Cloud. I. Filamentary Structures
We report Atacama Large Millimeter/submillimeter Array/Atacama Compact Array observations of a high-density region of the Corona Australis cloud forming a young star cluster, and the results of resolving internal structures. In addition to embedded Class
Kengo Tachihara +19 more
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Abundances of Chemical Elements in Open Star Clusters as Indicators of their Nature
Applying a compilled catalog, we find that the relative abundances of α-elements in open clusters and in field stars of the thin disk of the Galaxy show different dependencies on metallicity, age and parameters of their Galactic orbits.
Marsakov V. A. +3 more
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M. V. Penston +3 more
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Evidence for Spatially Distinct Galactic Dust Populations
We present an implementation of a Bayesian mixture model using Hamiltonian Monte Carlo techniques to search for the spatial separation of Galactic dust populations. Utilizing intensity measurements from the Planck High Frequency Instrument, we apply this
Corwin Shiu +7 more
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Chemical Composition of Interstellar Dust Clouds
Starpzvaigžņu gāzu-putekļu mākoņu ķīmiskais sastāvs. Kalvāns J., Zinātniskie vadītāji Dr.phys. Šmelds I., asoc. prof. Actiņš A.. Maģistra darbs. 55 lappuses, 9 attēli, 4 tabulas, 37 literatūras avoti. Latviešu valodā.
Kalvāns, Juris
core
Dark ice chemistry in interstellar clouds [PDF]
This thesis is largely an experimental study on the formation of solid-state simple and complex organic molecules in the H2O-rich and CO-rich ice phases of dense interstellar clouds and dark cores. Astronomical ice observations are also presented and are
Qasim, D.N.
core
We report 850 μ m continuum polarization observations toward the filamentary high-mass star-forming region NGC 2264, taken as part of the B -fields In STar forming Regions Observations large program on the James Clerk Maxwell Telescope. These data reveal
Jia-Wei Wang +156 more
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On the Stability of Interstellar Neutral Hydrogen Clouds at Large Z-heights
Galactic neutral hydrogen (H i ) data drawn from several large-scale surveys have been used to study 32 small clouds found between Galactic longitudes 70° and 140° and latitudes −20° and −45°.
G. L. Verschuur
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The Large Magellanic Cloud (LMC) exhibits vigorous high-mass star formation, including the H ii regions of 30 Dor, which is the most active site of star formation in the Local Group.
Rin I. Yamada +17 more
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Cloud-cloud collisions in the interstellar medium
Results are presented from time-dependent numerical simulations of cloud-cloud collisions in the interstellar medium. Special emphasis is placed on physically detailed models of cloud collisions. The numerical simulations include heating, cooling, thermal conductivity, self-gravity, and molecule formation; magnetic fields have been neglected.
openaire +1 more source

