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Dust Extinction from RF Regression of Interstellar Lines
Dust extinction is ubiquitous in the Universe and a challenge in the correction of the brightness and color in astronomical observations. Spectral... -
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The Impact of Dust on Cepheid and Type Ia Supernova Distances
Milky-Way and intergalactic dust extinction and reddening must be accounted for in measurements of distances throughout the universe. This work... -
Interstellar Absorption and Dust Scattering
The study of the interstellar medium (ISM) in the X-rays has entered a golden age with the advent of the X-ray observatories XMM-Newton and Chandra.... -
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Map** the Interstellar Dust with Near-Infrared Observations: An Optimized Multi-Band Technique
We generalize Lada et al. (1994) NICE technique to map dust column density through a molecular cloud to an optimized multi-band technique that can be... -
A Three-Dimensional Analytical Model of the Interstellar Extinction within the Nearest Kiloparsec
AbstractWe present a new version of our analytical model of the spatial interstellar extinction variations within the nearest kiloparsec from the...
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Attenuation of electromagnetic wave propagation in Martian dust storms
Mars dust storms can significantly affect the radio communication link. In this paper, we proposed a predictive model based on Rayleigh theory. The...
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Interstellar Absorption and Dust Scattering
The study of the interstellar medium (ISM) in the X-rays has entered a golden age with the advent of the X-ray observatories XMM-Newton and Chandra.... -
Dust in the Diffuse ISM
The nature of the dust in the dispersed interstellar medium is determined by various observational limitations, which we summarize with special... -
Newly formed dust within the circumstellar environment of SN Ia-CSM 2018evt
Dust associated with various stellar sources in galaxies at all cosmic epochs remains a controversial topic, particularly whether supernovae play an...
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Dust in and Around the Heliosphere and Astrospheres
Interstellar dust particles were discovered in situ, in the solar system, with the Ulysses mission’s dust detector in 1992. Ever since, more...
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Dust scattered radiation in the galactic poles
We have modeled the diffuse background at the Galactic Poles in the far-ultraviolet (FUV: 1536 Å) and the near-ultraviolet (NUV: 2316 Å). The...
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Interstellar Extinction in Galactic Cirri in SDSS Stripe 82
AbstractWe have applied the method of star counts with Wolf diagrams to determine the interstellar extinction in five Galactic cirri in Sloan Digital...
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Extremely Red Galaxies: Dust Attenuation and Classification
The “extremely red galaxies” (ERGs) constitute a controversial population in deep near-IR surveys. Their extremely-red observed colours (I... -
The Role of Dust in GRB Afterglows
We show that the clumpy structure of star-forming regions can naturally explain the fact that 50-70% of GRB afterglows are optical “dark.” We also... -
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Decoupling of dust cloud and embedding plasma for high electron depletion in nanodusty plasmas
In recent years nanoparticles have become key technological products, e.g., as coatings with tunable optical gap in third generation solar cells, as...
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