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Titlebook: Light on Dark Matter; Proceedings of the F Frank P. Israel Conference proceedings 1986 D. Reidel Publishing Company, Dordrecht, Holland 198

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书目名称Light on Dark Matter
副标题Proceedings of the F
编辑Frank P. Israel
视频video
丛书名称Astrophysics and Space Science Library
图书封面Titlebook: Light on Dark Matter; Proceedings of the F Frank P. Israel Conference proceedings 1986 D. Reidel Publishing Company, Dordrecht, Holland 198
描述‘Light on Dark Matter‘, held from 10-14 June 1985 in the Dutch seaside resort of Noordwijk, was the first international conference devoted to the results of the all-sky survey by the US-Dutch-UK Infra-Red Astronomical Satellite (IRAS). As such, it was a hommage to the scientists, engineers and technicians who conceived, built and operated this extremely successful satellite. That this was generally felt to be the case, was proven by the large number of participants (over 200 from seventeen different nations), the li vely discussions, and the great variety of topics presented during the meeting. All this not withstanding a typical Dutch summer: gale-force winds, heavy cloud cover, and meter-high surf crashing onto a beach on which only the hardy ventur. ed. Most participants contented themselves by watching the lonely seagulls patrolling the North Sea coastline through the panoramic windows of the conference center. Parallel to the IRAS Conference, a Workshop on Infrared Properties of Interstellar Grains was organized by J. M. Greenberg of the Leiden Laboratory Astrophysics Group: a busy shuttling of participants between the Workshop room and the Main Conference Hall showed that man
出版日期Conference proceedings 1986
关键词CCD; astronomy; cosmology; galaxy; stars
版次1
doihttps://doi.org/10.1007/978-94-009-4672-9
isbn_softcover978-94-010-8577-9
isbn_ebook978-94-009-4672-9Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightD. Reidel Publishing Company, Dordrecht, Holland 1986
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Heliocentric Dependences of Zodiacal Emission, Temperature and Albedomodel-dependence is reduced, compared to the values averaged on the line-of-sight. The temperature probably does not exceed 250 K at the distance of the Earth. The albedo is found to decrease from ~ 0.08 at the distance of the Earth to ~ 0.06 at the distance of Mars.
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IRAS Intrinsic Colours of Hot Starscz (1979) models from the visual to 12 µm results in a 12 µm flux that is about 10 percent too low, and b) The energy distribution for hot stars from 0.4 to 12 µm cannot be described with a one-temperature blackbody.
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The Disc Structure and Mass Loss Rates of Be Starsree-free radiation from the disc. The density structures of the discs suggest that matter is accelerated outwards. The mass loss rates are of the order 7 10. to 2 10. M./yr, i.e. a factor 100 larger than derived from UV resonance lines (Snow, 1981).
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