Results 121 to 130 of about 430,768 (202)
Novel algorithms for the understanding of the chemical cosmos [PDF]
Molecular data from the interstellar medium (ISM) contain information that holds the key to understanding our chemically controlled cosmos and to unlocking the secrets of our universe.
Makrymallis, A
core
Despite the pervasive nature of interstellar dust and its impact on nearly all observations, most dust corrections employ line-of-sight averages over large angular scales.
Jordan A. Bartlett, Henry A. Kobulnicky
doaj +1 more source
We present a catalog of individual stellar and dust extinction properties along close to 500,000 sight lines in the southwest bar of the Small Magellanic Cloud (SMC). The catalog is based on multiband Hubble Space Telescope photometric data spanning near-
Petia Yanchulova Merica-Jones +10 more
doaj +1 more source
Galactic interstellar dust extinction effect on jets Emitted from galactic nuclei
AGN jet research is essential to comprehending galaxy evolution and the interac tions between supermassive black holes and their host environments.
Tolu Biressa +2 more
core
Grain growth, optical polarisation, and extinction in interstellar clouds [PDF]
Increases in the wavelength of maximum polarization and the ratio of total to selective extinction are generally assumed to be the result of grain growth in interstellar clouds.
Jones, A. P.
core
We investigate the radial dependence of the scaling relations of dust attenuation in nearby galaxies using integral field spectroscopy data from MaNGA.
Niu Li, Cheng Li
doaj +1 more source
The Spheroidal Analog Method for Modeling Irregular Porous Aggregates
It is shown that the optical properties of an irregular porous grain with effective radius a _eff ≲ 3 λ (where λ is the wavelength) can be well approximated by a “spheroidal analog”: a spheroid with appropriate axial ratio and size, with a dielectric ...
B. T. Draine
doaj +1 more source
Dust in the small Magellanic cloud. 1: Interstellar polarization and extinction data [PDF]
The typical extinction curve for the Small Magellanic Cloud (SMC), in contrast to that for the Galaxy, has no bump at 2175 A and has a steeper rise into the far ultraviolet.
Piirola, V. +3 more
core
Dust in and Around the Heliosphere and Astrospheres. [PDF]
Sterken VJ +9 more
europepmc +1 more source
Dust extinction-curve variation in the translucent interstellar medium is driven by PAH growth
11 pages, 6 figures, submitted on October 30 ...
Zhang, Xiangyu +2 more
openaire +2 more sources

