標(biāo)題: Titlebook: Astronomie spatiale infrarouge, aujourd‘hui et demain Infrared space astronomy, today and tomorrow; 3-28 August 1998 F. Casoli,J. Lequeux,F [打印本頁] 作者: tricuspid-valve 時間: 2025-3-21 17:48
書目名稱Astronomie spatiale infrarouge, aujourd‘hui et demain Infrared space astronomy, today and tomorrow影響因子(影響力)
書目名稱Astronomie spatiale infrarouge, aujourd‘hui et demain Infrared space astronomy, today and tomorrow影響因子(影響力)學(xué)科排名
書目名稱Astronomie spatiale infrarouge, aujourd‘hui et demain Infrared space astronomy, today and tomorrow網(wǎng)絡(luò)公開度
書目名稱Astronomie spatiale infrarouge, aujourd‘hui et demain Infrared space astronomy, today and tomorrow網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Astronomie spatiale infrarouge, aujourd‘hui et demain Infrared space astronomy, today and tomorrow被引頻次
書目名稱Astronomie spatiale infrarouge, aujourd‘hui et demain Infrared space astronomy, today and tomorrow被引頻次學(xué)科排名
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書目名稱Astronomie spatiale infrarouge, aujourd‘hui et demain Infrared space astronomy, today and tomorrow年度引用學(xué)科排名
書目名稱Astronomie spatiale infrarouge, aujourd‘hui et demain Infrared space astronomy, today and tomorrow讀者反饋
書目名稱Astronomie spatiale infrarouge, aujourd‘hui et demain Infrared space astronomy, today and tomorrow讀者反饋學(xué)科排名
作者: Liberate 時間: 2025-3-21 22:49
Some Quantitative Aspects of Galactic and Extragalactic Infrared Astronomy,Two types of infrared astrophysical problems have been intensively studied in recent years. The first is an investigation of primary coolants. The second is the nature of the diffuse extragalactic infrared background radiation.作者: 易改變 時間: 2025-3-22 03:37 作者: 鋼筆尖 時間: 2025-3-22 06:21
https://doi.org/10.1007/3-540-45573-6Cosmology; Dark Matter; Data Analysis; Galactic Structure; Infrared Astronomy; Stellar Structure; astronom作者: 諂媚于性 時間: 2025-3-22 09:43 作者: 壓倒 時間: 2025-3-22 14:15 作者: 畸形 時間: 2025-3-22 17:52 作者: Anhydrous 時間: 2025-3-22 22:12 作者: 易怒 時間: 2025-3-23 02:25
Fluorescence methods in polymer science,1995 November 17 and ended its life in May, 1998. It operated in the 2.5 – 18 μm range, and was developed by the ISOCAM consortium lead by the French Service d’Astrophysique of CEA Saclay. This paper reviews different algorithms which can be used for the calibration and analysis of ISOCAM data.作者: Mystic 時間: 2025-3-23 06:12
Michio Kurata,Walter H. Stockmayermmunity, covered the wavelength range from 2.5 – 240 μm at a wide variety of spectral and spatial resolutions and was operational between November 1995 and April 1998. The ISO data archive opened to the community in December 1998, at URL “www.iso.vilspa.esa.es”. The paper summarises the design and i作者: Bumble 時間: 2025-3-23 12:44
Fluorescence methods in polymer science,1995 November 17 and ended its life in May, 1998. It operated in the 2.5 – 18 μm range, and was developed by the ISOCAM consortium lead by the French Service d’Astrophysique of CEA Saclay. This paper reviews different algorithms which can be used for the calibration and analysis of ISOCAM data.作者: Derogate 時間: 2025-3-23 16:57 作者: 運動的我 時間: 2025-3-23 20:13 作者: nonradioactive 時間: 2025-3-23 23:20
L. E. Coleman Jr.,N. A. Meinhardtnd, possibly, of planets. Mostly, I will use simple theoretical arguments, which provide the framework for the understanding of the various stages that currently go under the definition of star formation. In some cases, I will describe briefly the observational techniques and results that have contr作者: 小口啜飲 時間: 2025-3-24 03:04 作者: Femine 時間: 2025-3-24 08:04 作者: Hdl348 時間: 2025-3-24 12:02 作者: Exhilarate 時間: 2025-3-24 16:37
https://doi.org/10.1007/BFb0050498ations for faint galaxy counts are recalled. The physical properties and spectral energy distributions of the dust that is responsible for the IR/submm emission are briefly described. The results of the ISOCAM and ISOPHOT deep surveys at 15 μm and 175 μm are reviewed, with those of the SCUBA deep su作者: 剛毅 時間: 2025-3-24 20:28 作者: insurgent 時間: 2025-3-25 01:57 作者: hair-bulb 時間: 2025-3-25 06:36
Cosmology with ISO,n with the so—called semi—analytic approach of galaxy formation are outlined. A preview of survey capabilities with forthcoming instruments after ISO shows that our knowledge of the “optically—dark” side of the universe should increase rapidly.作者: chemoprevention 時間: 2025-3-25 11:13
0924-8099 quality lectures should attract a wide audience..Includes suThis book brings together the lectures given at the Les Houches summer school "Infrared space astronomy, today and tomorrow". It gives a wide overview of infrared astronomy, a wavelength domain crucial for studies of the solar system, stars作者: 火海 時間: 2025-3-25 13:53
Fortschritte der Hochpolymeren-Forschungre and how stars make atoms heavier than helium: such questions have occupied the minds of astrophysicists in the first 2/3 of this century and the satisfactory answers to all this questions is undoubtedly one of the major successes of astrophysics in this century.作者: fiscal 時間: 2025-3-25 19:01
Stars and Galactic Structure,re and how stars make atoms heavier than helium: such questions have occupied the minds of astrophysicists in the first 2/3 of this century and the satisfactory answers to all this questions is undoubtedly one of the major successes of astrophysics in this century.作者: entitle 時間: 2025-3-25 22:59
Conference proceedings 2000 of infrared astronomy, a wavelength domain crucial for studies of the solar system, stars at the beginning and end of their lives, interstellar matter and galaxies at all distances. Recent developments in observational techniques have been tremendous. The first contributions give an introduction to作者: REIGN 時間: 2025-3-26 01:58
Overview of the ISO Mission,n-orbit performance of the satellite and its four scientific instruments, the operational scenario and some of the scientific highlights. It then focusses on ISO’s legacy to the astronomical community, giving an overview of the ISO data archive, its contents, access methods, available software tools and overall documentation.作者: allergen 時間: 2025-3-26 07:46 作者: 水土 時間: 2025-3-26 10:10 作者: DAFT 時間: 2025-3-26 13:51 作者: prediabetes 時間: 2025-3-26 19:42
L. E. Coleman Jr.,N. A. Meinhardtibuted to our knowledge of the processes in question, with particular emphasis on the ISO contributions. This order, . from theory to observations, has been chosen mostly for heuristic purposes. In reality, often observations have preceded and motivated theories, rather than vice-versa.作者: 聯(lián)想記憶 時間: 2025-3-26 21:54 作者: prick-test 時間: 2025-3-27 03:35
Dust in the Interstellar Medium,ion and composition. In dense clouds, dust is subject to processing involving grain growth through ice mantle formation and coagulation. Cloud collapse and star formation incorporate some of this dust into young stellar objects. Part of the dust will be included in a proto-planetary disc where it be作者: 群島 時間: 2025-3-27 05:43
Normal Galaxies in the Infrared,f normal galaxies has some very stable signatures, and other quite variable aspects. Much of this article is an attempt to understand what makes for stability in the spectrum, and what significance to attach to the variable parameters.作者: troponins 時間: 2025-3-27 11:06
Active Galaxies,at time were included. Radio-astronomical observations and infrared surveys with the Infrared Astronomical Satellite (IRAS) revealed new classes of active galaxies, like quasars and ultraluminous infrared galaxies (ULIRGs). Table 1 shows a classification of active galaxies based on their observation作者: myriad 時間: 2025-3-27 16:42 作者: Expostulate 時間: 2025-3-27 19:13 作者: 不怕任性 時間: 2025-3-28 00:07
O. Wichterle,J. ?ebenda,J. Králí?ekion and composition. In dense clouds, dust is subject to processing involving grain growth through ice mantle formation and coagulation. Cloud collapse and star formation incorporate some of this dust into young stellar objects. Part of the dust will be included in a proto-planetary disc where it be作者: diabetes 時間: 2025-3-28 04:38
O. Wichterle,J. ?ebenda,J. Králí?ekf normal galaxies has some very stable signatures, and other quite variable aspects. Much of this article is an attempt to understand what makes for stability in the spectrum, and what significance to attach to the variable parameters.作者: 身心疲憊 時間: 2025-3-28 07:34
https://doi.org/10.1007/BFb0050498at time were included. Radio-astronomical observations and infrared surveys with the Infrared Astronomical Satellite (IRAS) revealed new classes of active galaxies, like quasars and ultraluminous infrared galaxies (ULIRGs). Table 1 shows a classification of active galaxies based on their observation作者: floaters 時間: 2025-3-28 13:49 作者: G-spot 時間: 2025-3-28 14:51
Data Analysis with ISOCAM,1995 November 17 and ended its life in May, 1998. It operated in the 2.5 – 18 μm range, and was developed by the ISOCAM consortium lead by the French Service d’Astrophysique of CEA Saclay. This paper reviews different algorithms which can be used for the calibration and analysis of ISOCAM data.作者: GEN 時間: 2025-3-28 19:54
ISO Observations of Solar-System Objects,te have been performed on all classes of solar-system objects. Several important discoveries have been achieved, in particular with the Short-Wavelength Spectrometer. In spite of difficult observability constraints, spectra of Mars have been recorded with SWS and LWS. They have been used for a retri作者: 無節(jié)奏 時間: 2025-3-29 00:58
Stars and Galactic Structure,branches away from the main sequence; what white dwarfs and red giants are and why these differ from main-sequence stars; what the atomic abundances are and how stars make atoms heavier than helium: such questions have occupied the minds of astrophysicists in the first 2/3 of this century and the sa作者: neutralize 時間: 2025-3-29 03:18 作者: 思考而得 時間: 2025-3-29 08:07 作者: Suppository 時間: 2025-3-29 12:26
Normal Galaxies in the Infrared,nosity distribution. In such galaxies, the visible and ultraviolet is the only direct window onto the photospheres of stars, whereas the rest of the spectrum reflects reprocessed light from stars (Fig. 1). Dust in the interstellar medium reprocesses part of the stellar luminosity into infrared emiss
