Results 101 to 110 of about 834,499 (261)
A set of diffuse interstellar clouds in the inner Galaxy within a few hundred pc of the Galactic plane has been observed at an angular resolution of ~1 arcmin combining data from the NRAO Green Bank Telescope and the Very Large Array.
Dickey, John M. +3 more
core +2 more sources
Copernicus observations of C I and CO in diffuse interstellar clouds [PDF]
Copernicus was used to observe absorption lines of C I in its ground state and excited fine structure levels and CO toward 29 stars. We use the C I data to infer densities and pressures within the observed clouds, and because our results are of higher ...
Jenkins, E. B. +2 more
core +1 more source
The Spectral Energy Distribution of Self-gravitating Interstellar Clouds I. Spheres
We derive the spectral energy distribution (SED) of dusty, isothermal, self gravitating, stable and spherical clouds externally heated by the ambient interstellar radiation field.
Bernard J. P. +17 more
core +1 more source
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
doaj +1 more source
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
doaj +1 more source
The Fractal Dimension of Projected Clouds
The interstellar medium seems to have an underlying fractal structure which can be characterized through its fractal dimension. However, interstellar clouds are observed as projected two-dimensional images, and the projection of a tri-dimensional fractal
Beech M. +9 more
core +1 more source
Ice chemistry in the dense, cold interstellar medium (ISM) is probably responsible for the formation of interstellar complex organic molecules (COMs). Recent laboratory experiments performed at T ∼ 4 K have shown that irradiation of CO:N _2 ice samples ...
Rafael Martín-Doménech +3 more
doaj +1 more source
The Transition from Atomic to Molecular Hydrogen in Interstellar Clouds: 21 cm Signature of the Evolution of Cold Atomic Hydrogen in Dense Clouds [PDF]
P. F. Goldsmith, Di Li, Marko Krčo
openalex +1 more source
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
doaj +1 more source
Modelling the dust emission from dense interstellar clouds: disentangling the effects of radiative transfer and dust properties [PDF]
N. Ysard +23 more
openalex +1 more source

