Results 21 to 30 of about 2,805 (218)
On Graphite and Interstellar Extinction [PDF]
Mie scattering calculation to support theory that interstellar extinction is caused by graphite ...
T. P. Stecher, B. Donn
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High spatial resolution galactic 3D extinction mapping with IPHAS [PDF]
We present an algorithm (MEAD, for 'Mapping Extinction Against Distance') which will determine intrinsic (r' - i') colour, extinction, and distance for early-A to K4 stars extracted from the IPHAS r'/ i'/H alpha photometric data base.
R. A. H. Morris +46 more
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Interstellar extinction by composite grains [PDF]
Recent studies indicate that interstellar grains are composites of very small individual particles of silicates and carbon glued together into an aggregate.
J. S. Dobbie +3 more
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GALExtin: an alternative online tool to determine the interstellar extinction in the Milky Way [PDF]
International audienceEstimates of interstellar extinction are essential in a broad range of astronomical research. In the last decades, several maps and models of the large-scale interstellar extinction in the Galaxy have been published.
Arsenijevic, Vladan +8 more
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This review describes our current understanding of interstellar extinction. This differ substantially from the ideas of the 20th century. With infrared surveys of hundreds of millions of stars over the entire sky, such as 2MASS, SPITZER-IRAC, and WISE, we have looked at the densest and most rarefied regions of the interstellar medium at distances of a ...
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We have obtained accurate dust reddening from the far-ultraviolet to the mid-infrared for up to 5 million stars by the star-pair algorithm based on LAMOST stellar parameters along with Galaxy Evolution Explorer, Pan-STARRS 1, Gaia, Sloan Digital Sky ...
Ruoyi Zhang, Haibo Yuan
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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
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The 2175 Angstrom Interstellar Extinction Bump: Is the Wavelength Variable? [PDF]
The most striking characteristics of the mysterious 2175 Angstrom extinction bump, the strongest spectroscopic absorption feature seen on the interstellar extinction curve, are the invariant central wavelength and variable bandwidth: its peak position at
Yang, X. J., Wang, Qian, Li, Aigen
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An R V Map of the Milky Way Revealed by LAMOST
The total-to-selective extinction ratio, R _V , is a key parameter for tracing the properties of interstellar dust, as it directly determines the variation of the extinction curve with wavelength.
Ruoyi Zhang, Haibo Yuan, Bingqiu Chen
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Diamonds and the Interstellar Extinction Curve [PDF]
IT has been suggested1 that the interstellar extinction might be explained by assuming that the interstellar dust is composed of an appropriate size distribution of diamond particles. The imaginary part of the index of refraction of diamond increases sharply from near zero to about 1.0 at λ−1 = 5.0 µm−1, giving an albedo near unity in the visible and ...
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