Results 81 to 90 of about 104,518 (171)

Nanodust in the Interstellar Medium in Comparison to the Solar System

open access: yes, 2012
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
core   +1 more source

Theoretical Spectroscopic Study of Isopropyl Alcohol (CH3-CHOH-CH3)

open access: yesThe Astrophysical Journal
Accurate spectroscopic parameters of isopropyl alcohol, a volatile organic compound present on Earth and in extraterrestrial atmospheres, are provided.
Mohammed Salah   +3 more
doaj   +1 more source

Filamentary Hierarchies and Superbubbles: Galactic Multiscale Magnetohydrodynamic Simulations of Giant Molecular Cloud to Star Cluster Formation

open access: yesThe Astrophysical Journal
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
doaj   +1 more source

Variations of Interstellar Gas-to-dust Ratios at High Galactic Latitudes

open access: yesThe Astrophysical Journal
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
doaj   +1 more source

Possible interaction of interstellar particles with the solar and terrestrial environment [PDF]

open access: yes
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.
core   +1 more source

Physical Properties and H i-to-H2 Transition across Taurus Linear Edge

open access: yesThe Astrophysical Journal
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
doaj   +1 more source

The interface between the stellar wind and interstellar medium around R Cassiopeiae revealed by far-infrared imaging [PDF]

open access: bronze, 2009
T. UETA   +27 more
openalex   +1 more source

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