Results 91 to 100 of about 372,210 (210)
A 3.4 m absorption band in amorphous carbon: implications for interstellar dust [PDF]
W. W. Duley, D. A. Williams
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Interstellar Matter Structure along the Line of Sight to Cyg X-1
High-resolution spectra (R = 60 000) of Cyg X-1 = V1357 Cyg obtained with the NES echelle spectrograph of the Russian 6 meter telescope (3950–6690 Å) were used to study narrow interstellar absorption lines.
Bochkarev N. G. +3 more
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Fast, computer‐assisted detection of dust and debris impact craters on Stardust interstellar foils [PDF]
B. T. De Gregorio +5 more
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The first all-sky, high-resolution, 3D map of the optical extinction curve of the Milky Way revealed an unexpected steepening of the extinction curve in the moderate-density, “translucent” interstellar medium (ISM).
Xiangyu Zhang +2 more
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PILOT: a balloon-borne experiment to measure the polarized FIR emission of dust grains in the interstellar medium [PDF]
R. Misawa +57 more
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Dust/ice mixing in cold regions and solid-state water in the diffuse interstellar medium [PDF]
А. В. Потапов +3 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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COMPUTATIONAL STUDY OF INTERSTELLAR GLYCINE FORMATION OCCURRING AT RADICAL SURFACES OF WATER-ICE DUST PARTICLES [PDF]
Albert Rimola +2 more
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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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