Gaia-2MASS 3D maps of Galactic interstellar dust within 3 kpc [PDF]
Gaia stellar measurements are currently revolutionizing our knowledge of the evolutionary history of the Milky Way. 3D maps of the interstellar dust provide complementary information and are a tool for a wide range of uses.
R. Lallement +7 more
semanticscholar +1 more source
Diffuse interstellar bands as dust indicators: The contribution from 3D maps [PDF]
Three-dimensional (3D) distributions of the 862 nm diffuse interstellar band (DIB) carrier have been computed based on Gaia parallaxes and DIB catalogues, in parallel with 3D maps of dust extinction density.
R. Lallement, J. Vergely, N.L.J. Cox
semanticscholar +1 more source
INTERSTELLAR DUST GRAINS [PDF]
▪ Abstract This review surveys the observed properties of interstellar dust grains: the wavelength-dependent extinction of starlight, including absorption features, from UV to infrared; optical luminescence; infrared emission; microwave emission; optical,
B. Draine
semanticscholar +1 more source
Three-dimensional maps of interstellar dust in the Local Arm: using Gaia, 2MASS, and APOGEE-DR14 [PDF]
Context. Gaia data and stellar surveys open the way to the construction of detailed 3D maps of the Galactic interstellar (IS) dust based on the synthesis of star distances and extinctions. Dust maps are tools of broad use, also for Gaia-related Milky Way
R. Lallement +8 more
semanticscholar +1 more source
Interstellar extinction from photometric surveys: application to four high-latitude areas
Information on interstellar extinction and dust properties may be obtained from modern large photometric surveys data. Virtual Observatory facilities allow users to make a fast and correct cross-identification of objects from various surveys. It yields a
Malkov Oleg +13 more
doaj +1 more source
CMB Shadows: The Effect of Interstellar Extinction on Cosmic Microwave Background Polarization and Temperature Anisotropy [PDF]
We evaluate the degradation of the accuracy of the component separation between the cosmic microwave background (CMB) and foreground components caused by neglect of absorption of the CMB’s monopole component by the galactic interstellar matter.
Masashi Nashimoto +2 more
semanticscholar +1 more source
A Dynamical Constraint on Interstellar Dust Models from Radiative Torque Disruption [PDF]
Interstellar dust is an essential component of the interstellar medium (ISM) and plays critical roles in astrophysics. Achieving an accurate model of interstellar dust is therefore of great importance.
Thiem C. Hoang
semanticscholar +1 more source
The Near-infrared Extinction Law at High and Low Galactic Latitudes
The Milky Way dust extinction curve in the near-infrared (NIR) follows a power-law form, but the value of the slope, β _NIR , is debated. Systematic variations in the slope of the Milky Way UV extinction curve are known to be correlated with variations ...
Robert E. Butler, Samir Salim
doaj +1 more source
The Interstellar Dust Properties of Nearby Galaxies [PDF]
This article gives an overview of the constitution, physical conditions, and observables of dust in the interstellar medium of nearby galaxies. We first review the macroscopic, spatial distribution of dust in these objects and its consequences for our ...
F. Galliano +4 more
semanticscholar +1 more source
Interstellar Extinction and Elemental Abundances [PDF]
Elements in the interstellar medium (ISM) exist in the form of gas or dust. The interstellar extinction and elemental abundances provide crucial constraints on the composition, size, and quantity of interstellar dust.
Wenbo Zuo, Aigen Li, Gang Zhao
semanticscholar +1 more source

