標(biāo)題: Titlebook: Science with the Atacama Large Millimeter Array:; A New Era for Astrop Rafael Bachiller,José Cernicharo Conference proceedings 2008 Springe [打印本頁] 作者: 烹飪 時(shí)間: 2025-3-21 17:25
書目名稱Science with the Atacama Large Millimeter Array:影響因子(影響力)
書目名稱Science with the Atacama Large Millimeter Array:影響因子(影響力)學(xué)科排名
書目名稱Science with the Atacama Large Millimeter Array:網(wǎng)絡(luò)公開度
書目名稱Science with the Atacama Large Millimeter Array:網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Science with the Atacama Large Millimeter Array:被引頻次
書目名稱Science with the Atacama Large Millimeter Array:被引頻次學(xué)科排名
書目名稱Science with the Atacama Large Millimeter Array:年度引用
書目名稱Science with the Atacama Large Millimeter Array:年度引用學(xué)科排名
書目名稱Science with the Atacama Large Millimeter Array:讀者反饋
書目名稱Science with the Atacama Large Millimeter Array:讀者反饋學(xué)科排名
作者: Brocas-Area 時(shí)間: 2025-3-21 21:00 作者: infringe 時(shí)間: 2025-3-22 03:42
Alwyn Woottenssing the techniques developed in this area, which will have a significant effect on futuremedicine and healthcare, the book is a valuable resource for researchers, students, engineers, and professionals working in the fields of medical systems, medical technology, and intelligent systems..作者: atopic 時(shí)間: 2025-3-22 07:40 作者: MERIT 時(shí)間: 2025-3-22 11:25 作者: defuse 時(shí)間: 2025-3-22 15:15
R. Cesaroni Consequently, we regard intensity as Z coordinate and compute SI values within each slice. A computed SI represents the shape of intensity surface or the variation of intensity near to a target pixel. Furthermore, we also show the proposed method can be applied to nuclear segmentation with a differ作者: diathermy 時(shí)間: 2025-3-22 20:46
Philippe André,Patrick Hennebelle,Nicolas Perettodata quality. In order to reduce the patches without cells, we combined opening and closing operation with Otsu algorithm together. In addition, the hard negative method was also been used to remove false positives and balance positive and negative samples. Our method yields progressive sensitivity 作者: 傾聽 時(shí)間: 2025-3-22 23:55
Yuri Aikawaut a prototype of a proximity authentication system at medical institutions. The results showed that the mean length of time before the screen startup for electronic medical record terminals with and without a proximity authentication system was 5.89 and 12.28?s, respectively (p?
作者: 說明 時(shí)間: 2025-3-23 01:40
Debra?S. Shepherdut a prototype of a proximity authentication system at medical institutions. The results showed that the mean length of time before the screen startup for electronic medical record terminals with and without a proximity authentication system was 5.89 and 12.28?s, respectively (p?
作者: inflate 時(shí)間: 2025-3-23 06:47
M. Guélin,N. Brouillet,J. Cernicharo,F. Combes,A. Wootenment in Russia helps us better appreciate the challenges and opportunities facing emerging social forces in formerly communist party-led states. In this chapter, we explore how the Russian women’s movement is affected by the changing political-economic environment and by international contacts and r作者: cajole 時(shí)間: 2025-3-23 13:26
C. L. Brogan,T. R. Hunter,R. Indebetouw,C. J. Chandler,Y. L. Shirley,R. Rao,A. P. Sarmament in Russia helps us better appreciate the challenges and opportunities facing emerging social forces in formerly communist party-led states. In this chapter, we explore how the Russian women’s movement is affected by the changing political-economic environment and by international contacts and r作者: 嘲笑 時(shí)間: 2025-3-23 14:51
Claudia Comito,Peter Schilke,Ulrike Endesfelder,Izaskun Jiménez-Serra,Jesus Martín-Pintadoment in Russia helps us better appreciate the challenges and opportunities facing emerging social forces in formerly communist party-led states. In this chapter, we explore how the Russian women’s movement is affected by the changing political-economic environment and by international contacts and r作者: right-atrium 時(shí)間: 2025-3-23 18:23 作者: Myocarditis 時(shí)間: 2025-3-24 00:15 作者: IST 時(shí)間: 2025-3-24 04:19 作者: 緩解 時(shí)間: 2025-3-24 07:20
D. C. Lis,M. Gerin,E. Roueff,T. G. Phillips,D. R. Poelman Gro?unternehmungen an die Grenzen des eigenen Ressourcen- und Kompetenzenpotentials sto?en. Trotz dieser deutlichen Entwicklung mangelt es jedoch an konzeptionellem und theoretischem Rüstzeug zur Erkl?rung ressourcenbasierter Innovationsprozesse im allgemeinen und netzwerkartiger Innovationsprozess作者: 染色體 時(shí)間: 2025-3-24 11:56
Leonardo Bronfmanadherence to WHO recommendations could be associated to an osteoporosis risk reduction of 3,7%. Conclusion: Machine Learning and Data Mining algorithms can help us identify key factors in preventing osteoporosis. Our analysis shows that complying to WHO guidelines for physical activity could have a 作者: Incommensurate 時(shí)間: 2025-3-24 18:04 作者: 正面 時(shí)間: 2025-3-24 20:23
Tetsuo Hasegawa,Takaaki Arai,Nobuyuki Yamaguchi,Fumio Sato,the ASTE teamnclusion, the evidence supports the use of exergames to improve quality of life and depressive symptoms in patients diagnosed with a severe mental disorder. Nevertheless, it is a poorly studied population, and more research is needed to provide adequate specific guidelines and recommendations on vir作者: 責(zé)問 時(shí)間: 2025-3-25 01:50 作者: 節(jié)省 時(shí)間: 2025-3-25 07:02
planet formation) with prospects to the revolutionary results to be obtained with ALMA. These topics, discussed with special emphasis on millimeter and sub-millimeter astronomy, are presented by some of the mo978-94-017-8484-9978-1-4020-6935-2作者: Optimum 時(shí)間: 2025-3-25 11:31 作者: PON 時(shí)間: 2025-3-25 13:27 作者: 爆炸 時(shí)間: 2025-3-25 18:05 作者: Thymus 時(shí)間: 2025-3-25 23:39
The physical conditions in the BHR71 outflows, shown to be bipolar. We also measure temperature enhancements in the lobes. The CO and methanol LVG modelling points to temperatures between 30 and 50?K in the two lobes. The methanol emission in the southern lobe bright knot is barely resolved with the APEX single-dish. ALMA will thus be a central作者: Nostalgia 時(shí)間: 2025-3-26 01:08
Conference proceedings 2008axies, the physics and chemistry of the interstellar medium, and the processes of star and planet formation) with prospects to the revolutionary results to be obtained with ALMA. These topics, discussed with special emphasis on millimeter and sub-millimeter astronomy, are presented by some of the mo作者: Rustproof 時(shí)間: 2025-3-26 04:26 作者: 披肩 時(shí)間: 2025-3-26 11:22
978-94-017-8484-9Springer Science+Business Media B.V. 2008作者: 惹人反感 時(shí)間: 2025-3-26 16:33 作者: ineffectual 時(shí)間: 2025-3-26 18:29
https://doi.org/10.1007/978-1-4020-6935-2ALMA; Astrophysics; Cosmology; Evolution; Galaxies; Radioastronomy; Redshift; Star Formation; Universe; molec作者: 空氣傳播 時(shí)間: 2025-3-26 21:49 作者: commonsense 時(shí)間: 2025-3-27 01:32
Star and planet-formation with ALMA: an overview,led imaging of the collapse of pre-stellar cores and measuring the accretion rate of matter onto deeply embedded protostars, to unravelling the chemistry and dynamics of high-mass star-forming clusters and high-spatial resolution studies of protoplanetary disks down to the 1?AU scale.作者: 同步左右 時(shí)間: 2025-3-27 08:57
Interstellar deuteroammonia,ll as .-deuterated ammonia and methanol. We review the current understanding of depletion and deuteration processes in cold, dense interstellar medium (ISM) and discuss the utility of deuteroammonia as a tracer of the physical conditions and kinematics of cold, dense gas.作者: VOK 時(shí)間: 2025-3-27 11:40 作者: NIP 時(shí)間: 2025-3-27 14:06
High resolution submillimeter observations of massive protostars, evolutionary stages coexisting in close proximity. In the presence of such complexity and multiplicity of sources, these data suggest that the interpretation of diagnostics such as kinematic velocity gradients and temperatures that are strongly dependent on spatial resolution should be approached cautiously.作者: Fibrillation 時(shí)間: 2025-3-27 21:06 作者: antidote 時(shí)間: 2025-3-28 01:29 作者: calamity 時(shí)間: 2025-3-28 04:04 作者: geriatrician 時(shí)間: 2025-3-28 06:45
APEX and ATCA observations of the southern hot core G327.3-0.6 and its environs,ith cm continuum observations, the data reveal like pearls on a string several stages of massive star formation, with likely the youngest stages hiding in the cold N.H. cores analysed with a multilevel study of the APEX and ATCA observations.作者: Insubordinate 時(shí)間: 2025-3-28 12:35
prospects with such a unique facility.Provides the science c.Currently under construction in the Andean Altiplano, Northern Chile, the Atacama Large Millimeter Array (ALMA) is the most ambitious astronomy facility under construction. ALMA is a radio interferometer composed of 54 antennas of 12 m dia作者: 出血 時(shí)間: 2025-3-28 14:44 作者: 參考書目 時(shí)間: 2025-3-28 22:49 作者: Anticoagulant 時(shí)間: 2025-3-29 01:05 作者: defendant 時(shí)間: 2025-3-29 04:49
,High-resolution mm interferometry and the search for?massive?protostellar disks: the case of Cep-A ually the result of the superposition of multiple hot-core-type objects, at least one of them ejecting an outflow at a small angle with respect to the line of sight. Together with the well-known large-scale outflow ejected by HW2, this setup makes for a very complex spatial and kinematic picture.作者: 痛苦一下 時(shí)間: 2025-3-29 09:23
SMA observations of the magnetic fields around a low-mass protostellar system,undred AU; gravity has overcome magnetic support and the magnetic field traces a clear hourglass shape. The magnetic field is substantially more important than turbulence in the evolution of the system and the initial misalignment of the magnetic and spin axes may have been important in the formation of the binary system.作者: 果核 時(shí)間: 2025-3-29 14:20 作者: JAMB 時(shí)間: 2025-3-29 15:41
High-mass star forming regions: An ALMA view,massive star formation. The impact of this new generation instrument will range from establishing the mass function of pre-stellar cores inside IR-dark clouds, to investigating the kinematics of the gas from which OB stars are built up, to assessing or ruling out the existence of circumstellar accretion disks in these objects.作者: 得意人 時(shí)間: 2025-3-29 19:45 作者: 天空 時(shí)間: 2025-3-30 01:32 作者: 凈禮 時(shí)間: 2025-3-30 08:00
ALMA capabilities for observations of continuum emission,ALMA’s sensitivity for continuum measurements is increased with the added feature of an 8 GHz instantaneous bandwidth. Taken together, these four factors provide unparalleled sensitivity in the millimeter/submillimeter wavelength range. With its great sensitivity and angular resolution, ALMA will tr作者: 仲裁者 時(shí)間: 2025-3-30 10:46
Star and planet-formation with ALMA: an overview,led imaging of the collapse of pre-stellar cores and measuring the accretion rate of matter onto deeply embedded protostars, to unravelling the chemistry and dynamics of high-mass star-forming clusters and high-spatial resolution studies of protoplanetary disks down to the 1?AU scale.作者: 卵石 時(shí)間: 2025-3-30 12:59 作者: 羊欄 時(shí)間: 2025-3-30 17:25
Early stages of star formation,nding of these deeply embedded stages is crucial to gain insight into the origin of stellar masses and binary systems. While the use of large single-dish (sub)millimeter radiotelescopes and existing interferometers has led to good progress on the overall density structure of isolated prestellar core作者: 系列 時(shí)間: 2025-3-31 00:28 作者: 詞匯記憶方法 時(shí)間: 2025-3-31 03:04
Molecular outflows observed with ALMA,erstanding of molecular outflows and the outflow/accretion connection. However, once the Atacama Large Millimeter Array (ALMA) is completed, it will provide a significant increase in sensitivity and resolution at millimeter and sub-millimeter wavelengths that will allow astronomers to address critic作者: entreat 時(shí)間: 2025-3-31 07:31
Unveiling the chemistry of hot protostellar cores with ALMA,several cores of size 10. AU, which have distinct spectral signatures. Complex molecules such as ethanol, vinyl cyanide and dimethyl ether show different distributions and their relative abundance varies from core to core by orders of magnitude. The molecular column densities derived in the cores al作者: CANDY 時(shí)間: 2025-3-31 11:58 作者: deriver 時(shí)間: 2025-3-31 14:58
,High-resolution mm interferometry and the search for?massive?protostellar disks: the case of Cep-A saic. This task is however observationally very challenging. A very interesting example is Cepheus A HW2. The properties of the molecular emission around this YSO seems to suggest the presence of a massive rotating disk (cf. Patel et al. in Nature 437:109, .). We have carried out sub-arcsec-resoluti作者: 植物學(xué) 時(shí)間: 2025-3-31 20:38 作者: innovation 時(shí)間: 2025-4-1 00:38
