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- W2026004080 abstract "view Abstract Citations (9) References (40) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Rocket observations of the Orion reflection nebulosity in the range 130-200 nanometers and scattering properties of dust grains in the far-ultraviolet. Onaka, T. ; Sawamura, M. ; Tanaka, W. ; Watanabe, T. ; Kodaira, K. Abstract Vacuum ultraviolet surface brightness maps of the southern part of the Orion region at the wavelengths 195.1, 179.6, 164.0, 148.4, and 132.8 nm were obtained by a rocket experiment. Large-scale bright nebulosity and a ridge structure in the western circumference of the Orion regions are clearly seen in these contour maps. Simple analysis shows that the observations can be explained by a front-dust-layer model, in which the diffuse light arises from the starlight scattered by dust grains in front of the stars, as well as by a back-dust-layer model, where dust grains behind the stars scatter the starlight to produce the diffuse nebulosity. A detailed discussion of the far-ultraviolet scattering properties of the dust grains in the observed region is included. Publication: The Astrophysical Journal Pub Date: December 1984 DOI: 10.1086/162696 Bibcode: 1984ApJ...287..359O Keywords: Interstellar Matter; Orion Nebula; Reflection Nebulae; Ultraviolet Astronomy; Astronomical Maps; Backscattering; Far Ultraviolet Radiation; Forward Scattering; Ridges; Spatial Distribution; Astrophysics full text sources ADS | data products SIMBAD (1)" @default.
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- W2026004080 date "1984-12-01" @default.
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- W2026004080 title "Rocket observations of the Orion reflection nebulosity in the range 130-200 nanometers and scattering properties of dust grains in the far-ultraviolet" @default.
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