Results 11 to 20 of about 418,445 (289)

Low Arabian dust extinction‐to‐backscatter ratio [PDF]

open access: yesGeophysical Research Letters, 2013
Compared to typical values of 50–60 sr of the extinction‐to‐backscatter ratio (lidar ratio) at 532 nm of western Saharan mineral dust, low dust lidar ratios from 33.7±6.7 to 39.1±5.1 sr were derived from polarization lidar observations at Limassol, Cyprus (34°N, 33°E) during an outbreak of Arabian dust mainly from Syria in September 2011, indicated by ...
R. E. Mamouri   +5 more
openaire   +3 more sources

DIBs, Interstellar Dust, and Extinction [PDF]

open access: yesProceedings of the International Astronomical Union, 2013
AbstractThe relationship between DIBs and dust is still unknown. The correlation between reddening and DIB strength means that the DIBs are mixed in with the dust and gas in interstellar clouds. The DIBs are relatively stronger in the diffuse interstellar medium than in dense clouds.
Clayton, G. C.
openaire   +3 more sources

On the Variation of Interstellar Dust Extinction [PDF]

open access: yes
Dust obscures astronomical observations and plays a important role in the evolution of galaxies. Mapping dust in three dimensions not only allows accurate correction of observations but also constrains the evolution of the interstellar medium (ISM). Extinction is the central observable to trace the density and properties of dust, and is widely employed
Zhang, Xiangyu
openaire   +3 more sources

Extinction and dust properties in a clumpy medium [PDF]

open access: yesAstronomy & Astrophysics, 2015
(abridged) The dust content of the universe is primarily explored via its interaction with stellar photons, producing interstellar extinction. However, owing to the physical extension of the observing beam, observations may detect scattered photons, resulting in a change in the observed (or effective) extinction, depending on the spatial distribution ...
Scicluna, P., Siebenmorgen, R.
openaire   +4 more sources

NEW ULTRAVIOLET EXTINCTION CURVES FOR INTERSTELLAR DUST IN M31 [PDF]

open access: yesThe Astrophysical Journal, 2015
ApJ, in press, 9 pages, 5 ...
Geoffrey C. Clayton   +6 more
openaire   +5 more sources

Limits on Dust Extinction in B3 QSOS

open access: yesAstrophysics and Space Science, 2001
Peer ...
Benn, C.R.   +4 more
openaire   +4 more sources

Modeling galactic extinction

open access: yesAtti della Accademia Peloritana dei Pericolanti : Classe di Scienze Fisiche, Matematiche e Naturali, 2011
We present a model for interstellar extinction dust, in which we assume a bimodal distribution of extinction carriers, a dispersion of core-mantle grains, supplemented by a collection of PAHs in free molecular form.
C. Cecchi-Pestellini   +7 more
doaj   +2 more sources

The extinction by dust in the outer parts of spiral galaxies

open access: yesAstronomy & Astrophysics, 1995
To investigate the distribution of dust in Sb and Sc galaxies we have analyzed near-infrared and optical surface photometry for an unbiased sample of 37 galaxies. Since light in the $K$-band is very little affected by extinction by dust, the $B-K$ colour is a good indicator of the amount of extinction, and using the colour-inclination relation we can ...
Peletier, R. F.   +5 more
core   +5 more sources

Dust extinction map of the Galactic plane based on the VVV survey data

open access: yes, 2022
Dust extinction is one of the most reliable tracers of the gas distribution in the Milky Way. The near-infrared (NIR) Vista Variables in the Via Lactea (VVV) survey enables extinction mapping based on stellar photometry over a large area in the Galactic ...
Kainulainen, Jouni   +4 more
core   +1 more source

A striking relationship between dust extinction and radio detection in DESI QSOs: evidence for a dusty blow-out phase in red QSOs [PDF]

open access: yes, 2023
We present the first eight months of data from our secondary target programme within the ongoing Dark Energy Spectroscopic Instrument (DESI) survey. Our programme uses a mid-infrared and optical colour selection to preferentially target dust-reddened ...
A Brodzeller   +85 more
core   +1 more source

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