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Interstellar polarization - Magnetite dust
The polarization and extinction properties of magnetite, or Fe$sub 3$O$sub 4$, dust grains are calculated based on indirect evidence that magnetite grains might be the interstellar polarizers. The extinction and phase-lag cross sections of magnetite grains are calculated using a computer method for nonspherical grains.
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INTERSTELLAR SILICATE ANALOGS FOR GRAIN-SURFACE REACTION EXPERIMENTS: GAS-PHASE CONDENSATION AND CHARACTERIZATION OF THE SILICATE DUST GRAINS [PDF]
T. Sabri +6 more
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Silicate Extinction Profile Based on the Stellar Spectrum by Spitzer/IRS
The 9.7 and 18 μ m interstellar spectral features, arising from the Si–O stretching and O–Si–O bending modes of amorphous silicate dust, are the strongest extinction features in the infrared.
Zhenzhen Shao, Biwei Jiang
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Modelling the dust emission from dense interstellar clouds: disentangling the effects of radiative transfer and dust properties [PDF]
N. Ysard +11 more
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Time Evolution of Optical Darkness in Gamma-Ray Burst Afterglow: The Case of GRB 240825A
Long-duration gamma-ray bursts (GRBs) are believed to occur in star-forming regions. The multiwavelength follow-up observations of the early afterglow of GRB 240825A provided insights into the evolution of the optical-to-X-ray spectral feature of the ...
Rui-Zhi Li +6 more
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Interstellar Dust at the Magnetic Wall of the Heliosphere. II [PDF]
P. C. Frisch
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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
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Interstellar Dust—Reply to Duley's Criticisms [PDF]
N. C. Wickramasinghe, K. Nandy
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