Results 1 to 10 of about 2,211 (208)
Interstellar Dust in the Solar System
A fraction of the dust in the interstellar medium (ISM) enters the heliosphere and is measured in situ from spacecraft. This review surveys the in situ measurements and discusses a hence derived model of dust in the local interstellar cloud (LIC).
Íngrid Mann
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The Interstellar Dust Properties of Nearby Galaxies
International audienceThis article gives an overview of the constitution, physical conditions, and observables of dust in the interstellar medium of nearby galaxies.
Frédéric Galliano +2 more
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Some of the next articles are maybe not open access.
2022
<p>Rare presolar grains originating by condensation in circumstellar atmospheres are known from meteorites [1]. These escaped processing in the solar nebula and are identified via their extremely diverse isotopic composition [1,2]. However, it is uncertain if such grains are representative for dust from the interstellar medium (ISM) [3 ...
Mario Trieloff +19 more
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<p>Rare presolar grains originating by condensation in circumstellar atmospheres are known from meteorites [1]. These escaped processing in the solar nebula and are identified via their extremely diverse isotopic composition [1,2]. However, it is uncertain if such grains are representative for dust from the interstellar medium (ISM) [3 ...
Mario Trieloff +19 more
openaire +1 more source
The Interstellar Dust Experiment (IDEX) is a dust impact ionization Time-of-Flight (ToF) mass spectrometer launched onboard the Interstellar Mapping and Acceleration Probe (IMAP) on September 24, 2025. IMAP is in nominal science operations at the Sun-Earth Lagrange Point L1, with IDEX passively collecting cosmic dust grains at a cadence of roughly one ...
Rebecca Mikula +10 more
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Rebecca Mikula +10 more
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Ice Formation on the Surfaces of Interstellar Dust Grains: Chemical Processing of the Ice
2015Ice mantles on the surfaces of interstellar dust grains are detected in denser, cooler gas clouds in the interstellar medium. The ices are predominantly water ice, with significant amounts of other fairly simple molecular species. The parameters controlling the onset of ice deposition are not well understood. Laboratory experiments show that mixed ices
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The mid- and far-infrared range: radiation emission processes from interstellar dust and gas
2013The thermal-infrared wavelength region contains the spectral signatures of solid-state compounds as well as a variety of lines emitted by atoms and molecules in the gaseous state. Together, these signatures provide unique diagnostic probes of the physical and chemical conditions of the cool and dusty Universe.
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Dynamical charging of interstellar dust particles in the heliosphere
Advances in Space Research, 2023V V Izmodenov
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Perspectives on Interstellar Dust Inside and Outside of the Heliosphere
Space Science Reviews, 2008B T Draine
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Interstellar Dust and Extinction
Annual Review of Astronomy and Astrophysics, 1990John S Mathis
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