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Titlebook: Astrophysics and Space Science; Volume 255, 1997/199 John Dyson,Susan A. Lamb,P. A. Zaal Book 1998 Springer Science+Business Media New York

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期刊全稱Astrophysics and Space Science
期刊簡稱Volume 255, 1997/199
影響因子2023John Dyson,Susan A. Lamb,P. A. Zaal
視頻videohttp://file.papertrans.cn/164/163698/163698.mp4
圖書封面Titlebook: Astrophysics and Space Science; Volume 255, 1997/199 John Dyson,Susan A. Lamb,P. A. Zaal Book 1998 Springer Science+Business Media New York
影響因子The successful launch on November 17, 1995 of ESA‘s Infrared Space Observatory (ISO) by means of an Ariane 4 carrier, has set in motion a true revolution in quantitative infrared astronomy. For the first time since the very successful IRAS mission in 1983, the astronomical community has uninterrupted access to the infrared part of the electromagnetic spectrum. The four focal plane instruments on board of ISO ( the camera ISOCAM, the photometerjcamera ISOPHOT, and the short and long wavelength spec- trographs ISO-SWS and ISO-LWS), perform very well and live up to the high expectations all of us had at launch. In the spring of 1996, Thijs de Graauw (principal investigator of the SWS) first suggested the idea to organize a conference dedicated to ISO re- sults in the area of stars and circumstellar matter, and coined the title ISO ‘s View on Stellar Evolution. At the first scientific meeting to highlight some of the early ISO results which was held in May of 1996 at ESA‘s laboratory ESTEC in Noordwijk, the Netherlands, the conference was announced and a preliminary science organizing committee was formed. The conference was held from July 1 to 4, 1997, in conference centre de Leeuwenh
Pindex Book 1998
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https://doi.org/10.1007/978-1-4302-0308-7rina spiral arm at a distance of 2.2 kpc (Chini et al., 1980). The cloud core M17-North is a dust condensation located 10′ north of the exciting stars of M17. It was investigated only by low-resolution studies of the whole cloud complex (e.g. Gatley et al. 1979; Wilson et al. 1979).
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The Camera Object and Flash Video,(FCS) with known output power. However, the short-period drifts of the C-100 detectors at the beginning of a measurement are on the same order of magnitude as the response to both faint source fluxes and the corresponding FCS power. Thus other techniques for calibrating ISOPHOT data on faint sources are sought.
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The Intermittently Embedded Herbig AE/BE StarsBe stars which are viewed edge-on to their polarimetrically identified dust and gas disks. The ISO SWS observations confirm the lack of a simple correlation between system age and the profile shape. Comparison with laboratory silicates suggests that much of the observed variation is due to different annealing histories of the grains.
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