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標(biāo)題: Titlebook: Atlas and Catalogue of Infrared Sources in the Magellanic Clouds; P. B. W. Schwering,F. P. Israel Book 1990 Kluwer Academic Publishers 199 [打印本頁]

作者: gratuity    時間: 2025-3-21 16:19
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作者: Ancestor    時間: 2025-3-21 22:05
The typology of the freestanding house,quently associated with dusty regions emitting primarily at far-infrared wavelengths (60 and 100 microns). We have cross-correlated the Infrared Catalogue with the catalogue of Hα nebulosities by Davies . (1976) and the dark cloud catalogues by Hodge (1972, 1974). Identifications and their quality (
作者: Glutinous    時間: 2025-3-22 04:06
https://doi.org/10.1007/978-3-0346-0463-5Add maps presented in the Atlas (Part 4). By comparison, the official IRAS Point Source Catalogue (PSC - see IRAS, 1989a) was derived from template fitting to individual one-dimensional survey scans. This method is unreliable in confused areas, such as the Clouds, mainly resulting in a higher degree
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作者: 廣口瓶    時間: 2025-3-22 10:57

作者: Diskectomy    時間: 2025-3-22 16:43

作者: 法律的瑕疵    時間: 2025-3-22 19:06
978-94-010-6728-7Kluwer Academic Publishers 1990
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作者: 忍耐    時間: 2025-3-23 11:01
interest in the skies, they noted the continuous presence of two cloud-like features, not far from the almost immediately Southern Pole. The first literature mention of these ‘clouds‘ was in the journal written in 1520 by the Italian navigator Pigafetta on the first circumnavigation of the globe by
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作者: 大范圍流行    時間: 2025-3-24 04:20
Atlas of Infrared Emission of the Magellanic Clouds, construct 2 Co-Added fields on the SMC, and 7 Co-Added fields on the LMC to complete coverage of infrared emission at the Cloud edges. The accompanying Table 4.1 lists individual field centers, and corresponding map page numbers, while Table 4.2 lists map properties of interest.
作者: 巫婆    時間: 2025-3-24 08:41
The Leiden-IRAS Magellanic Clouds Infrared Source Catalogues,entification with a PSC entry could be made, PSC positions are listed as these are the more accurate. For each source, we first list the peak intensity as well as the background emission level near the source. This is followed by a size estimate, based on the observed size and the nominal gaussian r
作者: 針葉類的樹    時間: 2025-3-24 12:07

作者: 織布機(jī)    時間: 2025-3-24 15:09

作者: 微生物    時間: 2025-3-24 22:02
Atlas and Catalogue of Infrared Sources in the Magellanic Clouds
作者: Radiculopathy    時間: 2025-3-25 00:54
Atlas and Catalogue of Infrared Sources in the Magellanic Clouds978-94-009-0537-5
作者: 偶然    時間: 2025-3-25 06:05

作者: frivolous    時間: 2025-3-25 08:28

作者: 莊嚴(yán)    時間: 2025-3-25 12:08
Infrared Source Identification Tables,quently associated with dusty regions emitting primarily at far-infrared wavelengths (60 and 100 microns). We have cross-correlated the Infrared Catalogue with the catalogue of Hα nebulosities by Davies . (1976) and the dark cloud catalogues by Hodge (1972, 1974). Identifications and their quality (
作者: arousal    時間: 2025-3-25 17:02
The Leiden-IRAS Magellanic Clouds Infrared Source Catalogues,Add maps presented in the Atlas (Part 4). By comparison, the official IRAS Point Source Catalogue (PSC - see IRAS, 1989a) was derived from template fitting to individual one-dimensional survey scans. This method is unreliable in confused areas, such as the Clouds, mainly resulting in a higher degree
作者: ACE-inhibitor    時間: 2025-3-25 22:10

作者: 全國性    時間: 2025-3-26 03:03
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