Results 61 to 70 of about 1,998 (179)
The Flattest Infrared Extinction Curve in Four Isolated Dense Molecular Cloud Cores
The extinction curve of interstellar dust in the dense molecular cloud cores is crucial for understanding dust properties, particularly size distribution and composition.
Jun Li +5 more
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Observation of Diffuse Galactic Light Near the Galactic Center with ONC-T on Board Hayabusa2
Diffuse Galactic light (DGL) is starlight scattered by interstellar dust. In visible wavelengths, earlier studies observed DGL toward regions of low optical depth in high Galactic latitude, and show marginal consistency with a theoretical model assuming ...
Kei Sano +23 more
doaj +1 more source
Properties of interstellar dust [PDF]
The reference abundance of the interstellar medium (the abundance of elements in gas + dust), until recently assumed to be solar, is discussed because of its great importance for the composition of dust. For some important elements (O, N, and probably more), three lines of reasoning (observed gas‐phase abundances, H II regions, and stellar abundances ...
openaire +1 more source
Properties of Interstellar Dust [PDF]
AbstractIn this review, the picture of the interstellar dust is outlined from the viewpoint of its role in galactic evolution. The modern concept of distinct dust populations is presented. The properties of the dust grains in the diffuse interstellar medium and in the molecular clouds are described.
openaire +1 more source
Thermodynamics of Giant Molecular Clouds: The Effects of Dust Grain Size
The dust grain size distribution (GSD) likely varies significantly across star-forming environments in the Universe, but its impact on star formation remains unclear. This ambiguity arises because the GSD interacts nonlinearly with processes like heating,
Nadine H. Soliman +2 more
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Imprints of the Local Bubble and Dust Complexity on Polarized Dust Emission
Using 3D dust maps and Planck polarized dust emission data, we investigate the influence of the 3D geometry of the nearby interstellar medium (ISM) on the statistics of the dust polarization on large ( $80^{\prime} $ ) scales.
George Halal +2 more
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Lifetimes of interstellar dust from cosmic ray exposure ages of presolar silicon carbide. [PDF]
Heck PR +9 more
europepmc +1 more source
The interstellar medium (ISM) consists of a diversity of structures across a range of spatial scales, intimately tied to galactic evolution. In this work, Fourier analysis is used to characterize the spatial structures of dust and polycyclic aromatic ...
Charlie Lind-Thomsen +2 more
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Mechanical Torque Disruption of Dust Grains Induced by Supernova Shock Waves
The feedback from massive stars drives the evolution of interstellar dust grains by altering their physical properties via a number of radiative and mechanical processes.
Sergio Martínez-González
doaj +1 more source

