標(biāo)題: Titlebook: Infrared Astronomy; Proceedings of the N Giancarlo Setti,Giovanni G. Fazio Conference proceedings 1978 D. Reidel Publishing Company, Dordre [打印本頁] 作者: FARCE 時間: 2025-3-21 18:36
書目名稱Infrared Astronomy影響因子(影響力)
書目名稱Infrared Astronomy影響因子(影響力)學(xué)科排名
書目名稱Infrared Astronomy網(wǎng)絡(luò)公開度
書目名稱Infrared Astronomy網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Infrared Astronomy被引頻次
書目名稱Infrared Astronomy被引頻次學(xué)科排名
書目名稱Infrared Astronomy年度引用
書目名稱Infrared Astronomy年度引用學(xué)科排名
書目名稱Infrared Astronomy讀者反饋
書目名稱Infrared Astronomy讀者反饋學(xué)科排名
作者: neologism 時間: 2025-3-21 22:14 作者: auxiliary 時間: 2025-3-22 03:00 作者: 輪流 時間: 2025-3-22 05:55
https://doi.org/10.1007/978-94-009-9815-5astronomy; astrophysics; interstellar matter; moon; planet; spectroscopy; star; star formation; stellar evol作者: calorie 時間: 2025-3-22 11:38 作者: deriver 時間: 2025-3-22 16:30
Theoretical Aspects of the Infrared Emission from HII RegionsTreatment of the subject of IR emission from HII regions will necessitate considerable discussion of the parameters and properties of dust grains. Therefore I feel that I should first justify why and how dust problems are strictly related to the IR astronomy and also why they are interesting.作者: 我的巨大 時間: 2025-3-22 18:51 作者: 玉米 時間: 2025-3-22 22:34 作者: wangle 時間: 2025-3-23 04:34
Infrared Astronomical SpectroscopySpectroscopic instruments are designed to divide radiation into its component wavelengths (or frequencies) and to provide the observer with a display of this information at high signal-to-noise ratio (SNR).作者: Ascendancy 時間: 2025-3-23 07:47
ine think?? gestellt worden. Die erste offene Frage bei dieser insgesamt r?tselhaften Angelegenheit ist, wieso Turing sie überhaupt selbst so stellte, denn er wich ihr sofort aus und ersetzte sie durch eine andere, nicht minder dunkle, n?mlich die, ob sich eine menschliche Schiedsrichterin oder ein 作者: countenance 時間: 2025-3-23 10:16 作者: FRAX-tool 時間: 2025-3-23 15:29
George Riekeenig beteiligt. Sieht man von diesem Sonderfall ab, so mu? das Verbindungsmaterial zun?chst eine ausreichende Bindef?higkeit gegenüber den Grundwerkstoffen besitzen, seine mechanischen Eigenschaften (Zug- bzw. Druckfestigkeit, Dehnung, Kerbschlagfestigkeit) müssen befriedigende Werte haben; daneben 作者: Antarctic 時間: 2025-3-23 19:36 作者: phlegm 時間: 2025-3-23 23:29
Charles Ryter allen Gesellschaftsbereichen sowie durch das Verlagern der Besch?ftigungen in die Informationsverarbeitungs- und Dienstleistungst?tigkeiten wahrnehmbar. Somit nahm auch das Bewusstsein in der Forschung, der Politik und der Arbeitswelt über die Ausma?e der Gesundheitsfolgen von der psychischen (Fehl作者: nutrition 時間: 2025-3-24 05:12
Bruce G. Elmegreen allen Gesellschaftsbereichen sowie durch das Verlagern der Besch?ftigungen in die Informationsverarbeitungs- und Dienstleistungst?tigkeiten wahrnehmbar. Somit nahm auch das Bewusstsein in der Forschung, der Politik und der Arbeitswelt über die Ausma?e der Gesundheitsfolgen von der psychischen (Fehl作者: antedate 時間: 2025-3-24 06:33 作者: 調(diào)整校對 時間: 2025-3-24 13:32 作者: 乞丐 時間: 2025-3-24 18:00 作者: 令人苦惱 時間: 2025-3-24 22:59
Infrared Observations of HII Regionse regions are associated with dense clouds of dust and gas, and there is strong evidence that star formation is also occurring. In the early 1970’s observations indicated that many HII regions radiate most of their energy at far-infrared wavelengths; therefore detailed infrared observations of these作者: 冬眠 時間: 2025-3-25 01:09
Physics and Astrophysics of Interstellar Dusteen changed. This is largely a result of the experience gained during the course. A number of results not presented in Erice have been included for completeness because there was inadequate time to do so during the course of lectures. I have tried to preserve the character of the lectures by limitin作者: 音的強(qiáng)弱 時間: 2025-3-25 04:49 作者: correspondent 時間: 2025-3-25 08:04
Star Formation and Related Topicssome of the problems involved and some results, mostly theoretical, of studies of star formation, concentrating on qualitative or “back-of-the-envelope” aspects. The first lecture will consider the collapse of individual protostars, as understood mainly from spherical collapse models; the second wil作者: 種植,培養(yǎng) 時間: 2025-3-25 11:41
Infrared Emission of the Galactic Center and Extragalactic Sources. In some cases, such as Seyfert galaxies, such processes are clearly occuring, but we are frustrated by the lack of detail that we can see in what is spatially an unresolved point. The Galactic Center would probably not hold our attention for long if we observed it from beyond the Local Group, but 作者: 壕溝 時間: 2025-3-25 16:58
Cosmological Aspects of Infrared and Millimetre Astronomytation that the infrared and submillimetre wavebands will be no exception to this rule. The aim of this short set of lectures is to discuss some of the more obvious aspects of particular interest to cosmology. Naturally, such predictions of what one expects to find in an unexplored waveband are haza作者: Nmda-Receptor 時間: 2025-3-25 21:39 作者: DEFT 時間: 2025-3-26 00:18
Infrared Astronomy from Space: A Review of Future Possibilitieso space is now set to occur in the early 1980’s. These will not strictly be the first infrared astronomical observations to be conducted from outside the earth’s atmosphere as there has been some military interest in this area for a number of years. A 2.7 μm equatorial sky survey is currently in pro作者: avarice 時間: 2025-3-26 04:26
Far Infrared Emission of Molecular Clouds and Star Formation in the Galaxy The flux received in a 0.5. beam is larger than that received in a 0.25. beam, showing that the source (say at ?5 kpc away) is ?50 pc in size, typical for a molecular cloud, and too large for an HII region. An estimate of the dust temperature is obtained from 2 color photometry (75–95 μm band and 1作者: 太空 時間: 2025-3-26 10:31
Shock Induced Star Formationcircumstances which can be classified broadly into two categories. Some gravitational instabilities seem to proceed “spontaneously” in a dense cloud, as a natural part of the cloud’s evolution: For example, a cloud may form in a state of high internal energy, either thermal, magnetic or turbulent in作者: enflame 時間: 2025-3-26 14:21
Four-Color Infrared Bolometer System for One-Meter Telescopedesigned, fabricated and tested by the Univsity of Palermo to be used as a focal plane instrument on the Center of Astrophysics/University of Arizona balloon-borne 102 cm telescope (Fazio et a1. 1974).作者: 混合 時間: 2025-3-26 17:01 作者: 運(yùn)動的我 時間: 2025-3-26 21:16
1389-2185 om July 9 - July 20, 1977 at the "E. Majorana" Centre for Scientific Culture. The course was fully supported by a grant from the NATO Advanced Study Institute Programme. It was attended by 82 participants from 15 countries. Even though the infrared portion of the electromagnetic spectrum covers an e作者: animated 時間: 2025-3-27 04:07
Infrared Observations of HII Regions regions could yield important new information on the evolution of pre-main sequence objects. Indeed, infrared observations obtained over the last seven years have confirmed these ideas. In these two lectures I will review what infrared observations have been made and what we have learned from them.作者: orthopedist 時間: 2025-3-27 07:55
Infrared Emission of the Galactic Center and Extragalactic Sourcesits proximity allows study on a scale completely unattainable for any other galactic nucleus. Thus, in the study of galaxies, it holds a unique place analogous to that of the sun in stellar astronomy.作者: 真繁榮 時間: 2025-3-27 11:51
Cosmological Aspects of Infrared and Millimetre Astronomyrdous but the apologia for such an exercise is that, if they encourage infrared astronomers to make the appropriate observations, they are likely to discover even more exciting things than one could have predicted.作者: defenses 時間: 2025-3-27 13:40
Shock Induced Star Formation origin and may become gradually unstable as this energy dissipates and the cloud cools radiatively. Similarly, some clouds may undergo molecular or grain-molecular reactions, thereby changing the balance between heating and cooling and eventually leading to gravita-tionally unstable regions.作者: 不真 時間: 2025-3-27 21:41
Physics and Astrophysics of Interstellar Dustmpleteness because there was inadequate time to do so during the course of lectures. I have tried to preserve the character of the lectures by limiting the mathematical detail and using physical or heuristic arguments to derive some of the formulae.作者: CHURL 時間: 2025-3-27 22:28
Star Formation and Related Topicse” aspects. The first lecture will consider the collapse of individual protostars, as understood mainly from spherical collapse models; the second will consider multidimensional collapse and the fragmentation problem; and the third will consider some aspects of star formation on a galactic scale.作者: NEEDY 時間: 2025-3-28 04:10
Far Infrared Emission of Molecular Clouds and Star Formation in the Galaxyl for a molecular cloud, and too large for an HII region. An estimate of the dust temperature is obtained from 2 color photometry (75–95 μm band and 115–196 μm band). The column density of the cloud is derived from .CO observations.作者: 共同生活 時間: 2025-3-28 07:32
Conference proceedings 1978- July 20, 1977 at the "E. Majorana" Centre for Scientific Culture. The course was fully supported by a grant from the NATO Advanced Study Institute Programme. It was attended by 82 participants from 15 countries. Even though the infrared portion of the electromagnetic spectrum covers an extensive i作者: GONG 時間: 2025-3-28 11:02
Conference proceedings 1978ralleled by an ever increasing interest of astronomers in infrared observations, leading to a number of ex- tremely important results in different branches of astronomy. This becomes evident when one realizes that in many astrophysical conditions most of the energy is found to be channeled into the 作者: 輕浮女 時間: 2025-3-28 15:25
Physics of Molecular Clouds from Millimeter Wave Line Observationsf magnitude and the production rate dominates with almost all hydrogen converted to H.. Since H. does not have a true continuum photodissociation at λ > 912 ?, the self shielding of the bound-bound-free process of the Lyman bands is critical to the distinction between atomic and molecular clouds.作者: 遭受 時間: 2025-3-28 19:39 作者: Forage飼料 時間: 2025-3-29 00:08 作者: OATH 時間: 2025-3-29 06:44
1389-2185 ferent branches of astronomy. This becomes evident when one realizes that in many astrophysical conditions most of the energy is found to be channeled into the 978-94-009-9817-9978-94-009-9815-5Series ISSN 1389-2185 作者: Seizure 時間: 2025-3-29 10:19
vor allem Computer, die sich als Autisten oder ukrainische Dreizehnj?hrige ausgeben, beim Turing-Test so gro?en Erfolg hatten. So jedenfalls zuletzt an der University of Reading 2014 erforscht. Manche Eltern freuten sich jedenfalls im Anschluss an diesen Erfolg, dass es ihnen gelungen sei, mit ihren作者: 分離 時間: 2025-3-29 14:16
Richard B. Larsonrken mu?, sind die Anforderungen sehr vielgestaltig, und es ist schwierig, wenn nicht unm?glich, sie alle vollst?ndig zu erfüllen. Teilweise durch Normung, teilweise durch anerkannte Regeln der Technik wurde versucht, diese anstehenden Fragen zu kl?ren. Es ist aber nicht zu vermeiden, da? viele dami作者: 令人悲傷 時間: 2025-3-29 15:57 作者: 幸福愉悅感 時間: 2025-3-29 20:52
Martin Harwitrken mu?, sind die Anforderungen sehr vielgestaltig, und es ist schwierig, wenn nicht unm?glich, sie alle vollst?ndig zu erfüllen. Teilweise durch Normung, teilweise durch anerkannte Regeln der Technik wurde versucht, diese anstehenden Fragen zu kl?ren. Es ist aber nicht zu vermeiden, da? viele dami作者: 特別容易碎 時間: 2025-3-30 03:04
Charles Ryterdie aktuelle kognitive Beanspruchung zu nutzen, ist nicht neu. Trotz der recht zahlreichen Studien sind dieErkenntnisse bis heute nicht hinreichend. Norman Re?ut widmet sich daher der Zielstellung, die aktuelle Erkenntnislage vom Zusammenhang der psychisch (mentalen) Belastung/ Beanspruchung und dem Lidschlag978-3-658-36051-1978-3-658-36052-8作者: 相符 時間: 2025-3-30 05:41 作者: 橢圓 時間: 2025-3-30 09:45
V. Daneu,C. Maxson,G. Peres,S. Serio,G. Vaianaren Liedkomponisten vor, dessen Produktion auf Grund von Eigenheiten, die in einem g?nzlich anderen Diskurs zu erl?utern und zu verstehen w?ren, als misslungen bezeichnet werden darf, noch m?chte ich eine Bewertung nach ?gut? und ?schlecht? suggerieren. Die Kategorie des Misslingens hat in diesem sp作者: antenna 時間: 2025-3-30 15:37
st geeignet gewesen, aber vielen Menschen h?tten die au?erordentlich zahlreichen Werke unterschiedlichster Gattungen .. Ein solches Urteil schloss einen Vergleich mit Johann Amons Zeitgenossen Wolfgang Amadé Mozart, Joseph Haydn und Antonio Rosetti oder Ludwig van Beethoven, Carl Maria von Weber und作者: 形狀 時間: 2025-3-30 19:28 作者: 圖畫文字 時間: 2025-3-30 22:30 作者: 流動性 時間: 2025-3-31 04:10 作者: 時代 時間: 2025-3-31 05:29
Directions for Future Research,solu-tion. Recently the entire zonal-scan procedure was com-puterized so that the distribution of the chemical mass or radioactivity along a chromatographic lane can be graphed by an electroplotter directed by the TLC computer program. The program gives a direct printout of area percent, recovery, a作者: FER 時間: 2025-3-31 09:36 作者: 性行為放縱者 時間: 2025-3-31 14:11 作者: 畫布 時間: 2025-3-31 20:23
Collective Learning in an Industry-Education-Research Test Bed in this collaborative industry–university environment. That process distilled a set of enacted principles. As a test bed for explicating the art and science of collectivity in creative practice, initial findings suggest the nature of fine-grained studies now needed to yield further insights, model and theorize collective learning.作者: PIZZA 時間: 2025-4-1 01:21 作者: Basal-Ganglia 時間: 2025-4-1 05:42
nfigurationen durch Vergleich mit den vorherigen Karten aber nach kurzer übung zu einem Gro?teil erkennen. Kleine Quadrate markieren besonders sch?ne Sternhaufen, Gasnebel und Galaxien, die mit einem Feldstecher und zum Teil sogar fürs blo?e Auge sichtbar sind.978-3-211-82233-3978-3-7091-9111-8作者: 花束 時間: 2025-4-1 07:30
Surveillance Camera and Its Calibration 7:49–66, 1951 [.]) summarizes popular camera calibration techniques during the period of 1880–1950s. Since the burgeoning of computer vision in 1960s, many modern camera calibration methods based on pinhole camera model have been proposed, which can be classified into two main categories: classic calibration and self-calibration.
