Results 41 to 50 of about 437,551 (293)

dustmaps: A Python interface for maps of interstellar dust

open access: yesJournal of Open Source Software, 2018
The dustmaps package provides a uniform Python interface for several commonly used maps of interstellar dust, including two-dimensional maps such as Schlegel, Finkbeiner, and Davis (1998), Planck Collaboration et al.
G. Green
semanticscholar   +1 more source

Computing the dust distribution in the bowshock of a fast moving, evolved star [PDF]

open access: yes, 2011
We study the hydrodynamical behavior occurring in the turbulent interaction zone of a fast moving red supergiant star, where the circumstellar and interstellar material collide.
Decin, Leen   +3 more
core   +7 more sources

Low temperature MIR to submillimeter mass absorption coefficient of interstellar dust analogues [PDF]

open access: yesAstronomy & Astrophysics, 2017
A wealth of data from the Herschel and Planck satellites and now from ALMA, revealing cold dust thermal emission, is available for astronomical environments ranging from interstellar clouds, cold clumps, circumstellar envelops, and protoplanetary disks ...
K. Demyk   +13 more
semanticscholar   +1 more source

One Relation for All Wavelengths: The Far-ultraviolet to Mid-infrared Milky Way Spectroscopic R(V)-dependent Dust Extinction Relationship

open access: yesThe Astrophysical Journal, 2023
Dust extinction is one of the fundamental measurements of dust grain sizes, compositions, and shapes. Most of the wavelength-dependent variations seen in Milky Way extinction are strongly correlated with the single parameter R ( V ) = A ( V )/ E ( B − V )
Karl D. Gordon   +6 more
doaj   +1 more source

The formation of peptide-like molecules on interstellar dust grains [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2018
Molecules with an amide functional group resemble peptide bonds, the molecular bridges that connect amino acids, and may thus be relevant in processes that lead to the formation of life.
N. Ligterink   +6 more
semanticscholar   +1 more source

Interstellar Dust

open access: yes, 2003
In the interstellar medium of the Milky Way, certain elements -- e.g., Mg, Si, Al, Ca, Ti, Fe -- reside predominantly in interstellar dust grains. These grains absorb, scatter, and emit electromagnetic radiation, heat the interstellar medium by photoelectric emission, play a role in the ionization balance of the gas, and catalyze the formation of ...
Michael A. Dopita, Ralph S. Sutherland
openaire   +3 more sources

Aspects of the Mass Distribution of Interstellar Dust Grains in the Solar System from In-Situ Measurements [PDF]

open access: yes, 1999
The in-situ detection of interstellar dust grains in the Solar System by the dust instruments on-board the Ulysses and Galileo spacecraft as well as the recent measurements of hyperbolic radar meteors give information on the properties of the ...
Baggaley   +30 more
core   +2 more sources

The galactic environment of the Sun [PDF]

open access: yes, 1999
The interstellar cloud surrounding the solar system regulates the galactic environment of the Sun and constrains the physical characteristics of the interplanetary medium.
Frisch, P. C.
core   +3 more sources

Dust in protoplanetary disks: observations*

open access: yesEPJ Web of Conferences, 2015
Solid particles, usually referred to as dust, are a crucial component of interstellar matter and of planet forming disks surrounding young stars. Despite the relatively small mass fraction of ≈1% (in the solar neighborhood of our galaxy; this number may ...
Waters L.B.F.M.
doaj   +1 more source

Dust absorption and scattering in the silicon K-edge [PDF]

open access: yes, 2019
The composition and properties of interstellar silicate dust are not well understood. In X-rays, interstellar dust can be studied in detail by making use of the fine structure features in the Si K-edge.
Costantini, E.   +7 more
core   +3 more sources

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