Nanodust in the Interstellar Medium in Comparison to the Solar System
Nanodust, which undergoes stochastic heating by single starlight photons in the interstellar medium, ranges from angstrom-sized large molecules containing tens to thousands of atoms (e.g.
Li, Aigen, Mann, Ingrid
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Theoretical Spectroscopic Study of Isopropyl Alcohol (CH3-CHOH-CH3)
Accurate spectroscopic parameters of isopropyl alcohol, a volatile organic compound present on Earth and in extraterrestrial atmospheres, are provided.
Mohammed Salah +3 more
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New insights into the interstellar medium of the dwarf galaxy IC 10: connection between magnetic fields, the radio–infrared correlation and star formation [PDF]
Aritra Basu +6 more
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Galactic fountains and outflows in star-forming dwarf galaxies: interstellar medium expulsion and chemical enrichment [PDF]
C. Melioli, F. Brighenti, A. D’Ercole
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There is now abundant observational evidence that star formation is a highly dynamical process that connects filament hierarchies and supernova feedback from galaxy-scale kiloparsec filaments and superbubbles to giant molecular clouds (GMCs) on 100 pc ...
Bo Zhao +4 more
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Dust emission in the diffuse interstellar medium from far-infrared to millimeter: new constraints from WMAP [PDF]
G. Lagache
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Variations of Interstellar Gas-to-dust Ratios at High Galactic Latitudes
Interstellar dust at high Galactic latitudes can influence astronomical foreground subtraction, produce diffuse scattered light, and soften the UV spectra of quasars.
J. Michael Shull, Georgia V. Panopoulou
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Possible interaction of interstellar particles with the solar and terrestrial environment [PDF]
The possibility for detection of interstellar particles in the earth's environment is considered on the basis of the passage of the solar system through the interstellar medium.
Greenberg, J. M.
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Physical Properties and H i-to-H2 Transition across Taurus Linear Edge
Studying the atomic-to-molecular transition is essential for understanding the evolution of the interstellar medium. The linear edge of the Taurus molecular cloud, clearly identified in the ^13 CO(1–0) intensity map, serves as an ideal site for ...
Ningyu Tang +7 more
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The interface between the stellar wind and interstellar medium around R Cassiopeiae revealed by far-infrared imaging [PDF]
T. UETA +27 more
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