標(biāo)題: Titlebook: Regions of Recent Star Formation; Proceedings of the S R. S. Roger,Peter E. Dewdney Conference proceedings 1982 D. Reidel Publishing Compan [打印本頁(yè)] 作者: 選民 時(shí)間: 2025-3-21 19:08
書目名稱Regions of Recent Star Formation影響因子(影響力)
書目名稱Regions of Recent Star Formation影響因子(影響力)學(xué)科排名
書目名稱Regions of Recent Star Formation網(wǎng)絡(luò)公開度
書目名稱Regions of Recent Star Formation網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Regions of Recent Star Formation被引頻次
書目名稱Regions of Recent Star Formation被引頻次學(xué)科排名
書目名稱Regions of Recent Star Formation年度引用
書目名稱Regions of Recent Star Formation年度引用學(xué)科排名
書目名稱Regions of Recent Star Formation讀者反饋
書目名稱Regions of Recent Star Formation讀者反饋學(xué)科排名
作者: Pessary 時(shí)間: 2025-3-21 23:16
G. Tenorio-Tagleion of skarn-hosted ore deposits. Most research on such settings has concentrated on mechanisms of melt intrusion and intrusive body formation, changes in temperature fields and stresses inside and in the vicinity of the intrusive body, the thermodynamic properties of melts, fluids and associated so作者: Amplify 時(shí)間: 2025-3-22 01:13 作者: 會(huì)議 時(shí)間: 2025-3-22 05:43 作者: 庇護(hù) 時(shí)間: 2025-3-22 11:20
H. E. Matthewsd optische Ver?nderungen vorzunehmen. Kurze Entwicklungszeiten, Leichtbau und Betriebsfestigkeitsprüfungen sind unabdingbar. Die damit verbundenen sehr komplexen Anforderungen lassen sich nur erfüllen, indem Simulationsprogramme für eine optimale Konstruktion und Fertigungsvorbereitung sowie moderne作者: locus-ceruleus 時(shí)間: 2025-3-22 15:16
A. Falchi,G. Tofani,R. H. Hartennerate and that pass through them. The recognition that such pro- cesses can profoundly affect the course of metamorphism has resulted in a number of recent papers and we consider that it is time for a review by some of the interested parties. We hope our selection of contributors provides an adequa作者: 枯萎將要 時(shí)間: 2025-3-22 20:52
T. J. Mazurektiven Zweipolen kann durch interne Rückkopplung ein negativer Widerstand auftreten, mit dem ein Resonator entd?mpft wird und somit ein Oszillator entsteht. Dieser Oszillator wird charakterisiert durch seine Amplitude und Frequenz sowie deren Fluktuationen, n?mlich Amplituden- und Frequenzrauschen. D作者: FRET 時(shí)間: 2025-3-23 00:41
J. R. Roy,R. Arsenault,G. Joncasndelten aktiven Zweipolen kann durch interne Rückkopplung ein negativer Widerstand auftreten, mit dem ein Resonator entd?mpft wird und somit ein Oszillator entsteht. Dieser Oszillator wird charakterisiert durch seine Amplitude und Frequenz sowie deren Fluktuationen, n?mlich Amplituden- und Frequenzr作者: admission 時(shí)間: 2025-3-23 02:02
George F. Mitchell,Terry J. Deveauhigh sensitivity is required. The need to optimize the fluorescence, both with respect to the total number of photons that can be extracted as well as to the fluorescence rate itself, is especially pronounced in applications regarding single molecule detection or fluorescence correlation spectroscop作者: semble 時(shí)間: 2025-3-23 06:44 作者: 等級(jí)的上升 時(shí)間: 2025-3-23 10:42
Johann Nittmannmical processes occurring in biological macromolecules over a large time span [2.1–2.3]. The application of FCS has enabled the retrieval of information on the properties of single biomolecules as distinguished from the collective properties of a whole molecular ensemble [2.4,2.5]. The FCS technique作者: 修飾 時(shí)間: 2025-3-23 17:46 作者: 陪審團(tuán)每個(gè)人 時(shí)間: 2025-3-23 20:57
Ronald L. Snell,Suzan EdwardsDNA. Our strategy was to extend the elegant concepts of fluctuation correlation spectroscopy to the dynamics of chemical interactions, which had not been accessible to previous fluctuation indicators such as quasi-elastic light scattering. Its first realization in studying interaction of a fluoresce作者: 陰謀 時(shí)間: 2025-3-24 00:02 作者: SENT 時(shí)間: 2025-3-24 03:44 作者: 長(zhǎng)處 時(shí)間: 2025-3-24 08:59 作者: 毗鄰 時(shí)間: 2025-3-24 13:07
High Velocity CO Emission around T Tauri Stars,T Tauri winds are detected via their interactions with ambient cloud material. The magnitude of the mass flows are calculated and dynamical effects on molecular clouds are discussed.作者: 支架 時(shí)間: 2025-3-24 17:51
Astrophysics and Space Science Libraryhttp://image.papertrans.cn/r/image/825488.jpg作者: 武器 時(shí)間: 2025-3-24 19:11
https://doi.org/10.1007/978-94-009-7778-5Galaxy; Supernova; galaxies; gravitation; gravity; star; star formation; stars; stellar作者: 河流 時(shí)間: 2025-3-25 00:20
Fine Structure Lines in HII Regions Interacting with Molecular Clouds,a balloon borne telescope with a Michelson interferometer system. The sources M42 and M17 have been mapped with a beam of 1.6’ FWHM. Physical quantities derived from these measurements are presented and some of the results are discussed.作者: Cosmopolitan 時(shí)間: 2025-3-25 04:38 作者: 慟哭 時(shí)間: 2025-3-25 10:49
Magnetic Fields and the Evolution of Shocked Gas Clouds,shock wave. The incident shock is assumed, a priori, to be driven by a spiral density wave. Results are presented for the flows which develop in the interstellar gas with magnetic field strength of 1μG and 3μG, respectively.作者: 萬(wàn)神殿 時(shí)間: 2025-3-25 14:39
Radiation-Hydrodynamics of HII Regions and Molecular Clouds,ur. The implosion of a cloud clump results in the formation of density enhancements that may eventually form low mass stars. The smaller globules produced may become Herbig-Haro objects, or maser sources.作者: 圖表證明 時(shí)間: 2025-3-25 16:27
High Velocity Gas in Molecular Clouds,ifted and blueshifted CO wings seen in this region are spatially separated indicating that this is another region of bi-polar mass outflow from a young stellar object. We compare this region to the other known regions of bi-polar mass outflow and discuss the implications of these energetic outflows.作者: assent 時(shí)間: 2025-3-25 23:44
978-94-009-7780-8D. Reidel Publishing Company, Dordrecht, Holland 1982作者: hematuria 時(shí)間: 2025-3-26 01:11
Regions of Recent Star Formation978-94-009-7778-5Series ISSN 0067-0057 Series E-ISSN 2214-7985 作者: NOVA 時(shí)間: 2025-3-26 05:55
0067-0057 ate of the four invited review papers. The subjects of these reviews are in the general areas of "Evolution of HII Regions", "Dynamical Interactions", "Chemistr978-94-009-7780-8978-94-009-7778-5Series ISSN 0067-0057 Series E-ISSN 2214-7985 作者: 攤位 時(shí)間: 2025-3-26 08:59 作者: 其他 時(shí)間: 2025-3-26 13:01
Conference proceedings 1982ted papers and the extent to which they addressed the subject matter. In the proceedings we have grouped these papers near the most appropriate of the four invited review papers. The subjects of these reviews are in the general areas of "Evolution of HII Regions", "Dynamical Interactions", "Chemistr作者: adhesive 時(shí)間: 2025-3-26 20:36
D. A. Naylor,R. Emery,B. Fitton,I. Furniss,R. E. Jennings,K. J. King作者: deface 時(shí)間: 2025-3-26 23:11 作者: Arthropathy 時(shí)間: 2025-3-27 02:36
G. Tenorio-Tagleand gas industry, and permeability experiments were generally conducted to 150°C and a few hundreds of atmospheres. The physical-chemical conditions of skarn formation, however, required knowledge of permeability to 600–700 °C and 1–2 kbar. In the works of ., ., and ., permeability measurements were作者: 創(chuàng)新 時(shí)間: 2025-3-27 08:39 作者: LAY 時(shí)間: 2025-3-27 13:10
R. H. Harten,M. Fellihrzeug bzw. das Bauteil frühzeitig analysierbar und ggf. folgend konstruktiv ?nderbar. Da ein Gro?teil der Versuchsst?nde und Belastungseinrichtungen einen oder mehrere hydraulische Antriebe haben, sollen einige von ihnen beispielhaft vorgestellt werden. Gleichzeitig sollen dem Ingenieur in der Prax作者: acquisition 時(shí)間: 2025-3-27 14:26 作者: syncope 時(shí)間: 2025-3-27 21:30
A. Falchi,G. Tofani,R. H. Harten. " We wish to thank D. Bird, S. Bohlen, D. Carmichael, G. Flowers, C. Foster, C. Graham, E. Perry, J. Selverstone, R. Tracy, J. Valley, and R. Wollast for their chapter reviews. Thanks are also due C. Cheverton for her editorial assistance, and the helpful staff at Springer-Verlag New York.作者: 小說 時(shí)間: 2025-3-28 01:56 作者: Irksome 時(shí)間: 2025-3-28 05:52 作者: 熱心 時(shí)間: 2025-3-28 08:21 作者: disrupt 時(shí)間: 2025-3-28 10:35 作者: Connotation 時(shí)間: 2025-3-28 15:18 作者: 震驚 時(shí)間: 2025-3-28 22:22 作者: itinerary 時(shí)間: 2025-3-29 01:39
Ronald L. Snell,Suzan Edwardsf the dynamics of molecular processes in and on living cells and tissues. Here I first report on the genesis of the concept and its realization in my laboratory at Cornell University. Then the evolution of FCS toward today‘s user-friendly status is discussed. Its maturation in some of our current re作者: bioavailability 時(shí)間: 2025-3-29 04:55 作者: ECG769 時(shí)間: 2025-3-29 10:45 作者: Baffle 時(shí)間: 2025-3-29 11:44 作者: 減震 時(shí)間: 2025-3-29 18:51 作者: Mammal 時(shí)間: 2025-3-29 23:16 作者: 不發(fā)音 時(shí)間: 2025-3-30 03:31
The Dynamical Evolution of an HII Region,e is no strong statistical evidence in support of the theory of successive star formation proposed by Elmegreen and Lada although there are several individual cases which do support it. This discrepancy is also discussed.作者: pus840 時(shí)間: 2025-3-30 04:13 作者: 遺忘 時(shí)間: 2025-3-30 08:54 作者: 無(wú)效 時(shí)間: 2025-3-30 15:47 作者: Rheumatologist 時(shí)間: 2025-3-30 17:02 作者: 約會(huì) 時(shí)間: 2025-3-30 22:43
Conference proceedings 1982and photochemical effects in regions showing clear evidence of on-going star formation. This is currently an are a of considerable research activity with much new observational material over the wavelength range from X-ray to radio. Furthermore, the field isbeginning to mature. No longer is molecula作者: 喊叫 時(shí)間: 2025-3-31 04:46
A Multi-Purpose Scanning Fabry-Perot Interferometer System,mator/camera optics. A Fabry lens forms an image of the primary on the photocathode of a Ga-As PM tube. Scanning of the Fabry-Pérot and data acquisition is done by a dedicated Rockwell AIM 65 microcomputer soon to be replaced by a HP-85 equipped with the HP-IB IEEE 488 interface bus.作者: Encapsulate 時(shí)間: 2025-3-31 06:39
0067-0057 dynamical and photochemical effects in regions showing clear evidence of on-going star formation. This is currently an are a of considerable research activity with much new observational material over the wavelength range from X-ray to radio. Furthermore, the field isbeginning to mature. No longer i作者: WATER 時(shí)間: 2025-3-31 11:24 作者: 多嘴 時(shí)間: 2025-3-31 14:42
HII Regions in Collapsing Massive Molecular Clouds,nted. Depending on the location of the exciting star, a champagne flow can occur concurrently with the central collapse of a nonrotating cloud. Partial evaporation of the cloud at a rate of about 0.005 M./yr results. When 100 0-stars are placed at the center of a freely falling cloud of 3 10. M. no 作者: Coordinate 時(shí)間: 2025-3-31 21:10
The Dynamical Evolution of an HII Region, of models of star formation and HII region evolution. Strong evidence is found in support of the ‘champagne flow’ model of HII region evolution. There is no strong statistical evidence in support of the theory of successive star formation proposed by Elmegreen and Lada although there are several in作者: 項(xiàng)目 時(shí)間: 2025-3-31 23:31
Radio Continuum Observations of W1,at λ11cm using the 100-m telescope in both total power and polarized radiation. The central part of the object also has been observed with the Westerbork Synthesis Radio Telescope at λ49, λ21, and λ6cm. In the light of these observations, the question of the existence of a non-thermal component of W作者: 費(fèi)解 時(shí)間: 2025-4-1 04:36 作者: investigate 時(shí)間: 2025-4-1 09:57 作者: 有發(fā)明天才 時(shí)間: 2025-4-1 12:01
HII Bubbles and Shocks in Molecular Clouds, is shown that density gradients in either the HII region or the exterior molecular cloud can naturally give supersonic gas speeds. Cases discussed include the swelling of uniform HII bubbles into clouds with decreasing densities, isothermal shock propagation within the ionized region, and homologou作者: 高貴領(lǐng)導(dǎo) 時(shí)間: 2025-4-1 14:31
