標(biāo)題: Titlebook: Lessons from the Local Group; A Conference in hono Kenneth Freeman,Bruce Elmegreen,Matthew Woolway Conference proceedings 2015 Springer Int [打印本頁] 作者: formation 時間: 2025-3-21 16:57
書目名稱Lessons from the Local Group影響因子(影響力)
書目名稱Lessons from the Local Group影響因子(影響力)學(xué)科排名
書目名稱Lessons from the Local Group網(wǎng)絡(luò)公開度
書目名稱Lessons from the Local Group網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Lessons from the Local Group被引頻次
書目名稱Lessons from the Local Group被引頻次學(xué)科排名
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書目名稱Lessons from the Local Group年度引用學(xué)科排名
書目名稱Lessons from the Local Group讀者反饋
書目名稱Lessons from the Local Group讀者反饋學(xué)科排名
作者: 去才蔑視 時間: 2025-3-21 21:40 作者: 類型 時間: 2025-3-22 02:48
P. C. van der Kruits necessary for agriculture to produce an irrigation system using modern technologies such as IoT and sensors which will improve the efficiency of water usage and further increase the crops yield that fulfil the food demand of humans and livestock. Hence, this project focuses on a smart irrigation s作者: 抵押貸款 時間: 2025-3-22 08:22
Ken C. Freemano eliminate the trial and error method when selecting the optimal controller parameter, we propose a PSO-based state feedback controller for the active suspension system. It is an intelligent-based method to determine state feedback gain controller by employing optimization technique using Particle 作者: 雪崩 時間: 2025-3-22 12:28 作者: CHYME 時間: 2025-3-22 13:27 作者: 1分開 時間: 2025-3-22 18:11
Jan Palou?,Soňa Ehlerovást-effectiveness, faster movements, and improved efficiency when compared to rigid beam structures. This research focuses on employing a proportional-integral-derivative (PID) controller to regulate the vibration level of a flexible beam structure. The tuning of this PID controller is crucial to max作者: emulsify 時間: 2025-3-22 22:18 作者: 口訣 時間: 2025-3-23 02:02 作者: 使混合 時間: 2025-3-23 06:31 作者: MANIA 時間: 2025-3-23 17:09 作者: 叫喊 時間: 2025-3-23 18:53 作者: Scintillations 時間: 2025-3-24 00:08 作者: 羽飾 時間: 2025-3-24 02:50 作者: Folklore 時間: 2025-3-24 07:07 作者: GLOSS 時間: 2025-3-24 12:08 作者: –FER 時間: 2025-3-24 15:28 作者: SLAG 時間: 2025-3-24 21:08
Steven R. Majewski,David R. Law,Sten Hasselquist,Guillermo Damkeging conditions, many distributed systems implement adaptive behavior. While simple adaptation through parameter tuning can only react to a limited range of conditions, a switch between different mechanisms at runtime enables broader adaptivity. However, distributed systems that switch mechanisms at作者: 江湖郎中 時間: 2025-3-25 01:46
,A Walk with Dr Allan Sandage—Changing the History of Galaxy Morphology, Forever, The author was the American astronomer E. P. Hubble. Several years ago, Dr Allan Sandage took one of us (David) on a walk from his office, to the library at the Carnegie Observatories in Pasadena. What Dr Sandage showed David, left him speechless.作者: nocturia 時間: 2025-3-25 03:55
Lessons From the Milky Way: The Kapteyn Universe, equilibrium between the gravitational field of the stars and their random motion and rotation. In the vertical direction Kapteyn’s results are substantially correct. Usually the Kapteyn Universe is described as being flawed due to neglect of interstellar absorption. Kapteyn was led to adopt this on作者: AMITY 時間: 2025-3-25 10:30
The Galactic Bulge, boxy/peanut-shaped bulge which we believe formed via instabilities of the disk rather than through mergers. The bulge of the Milky Way therefore appears to be a dynamical product of the early Galactic disk, without significant contamination from mergers with other galaxies. The instabilities are be作者: 變色龍 時間: 2025-3-25 13:50
The Galactic Bar,amical studies in the Gaia era. Here we discuss the pronounced peanut shape of the Galactic bulge that has resulted from recent star count analysis, in particular from the VVV survey. We also discuss the question whether the Milky Way has an inner disky pseudo-bulge, and show preliminary evidence fo作者: 弄皺 時間: 2025-3-25 18:44
The Challenge of Galactic Cartography: Lessons from the Milky Way, how or whether to include “historical” knowledge, based on traveler accounts, in their maps. I describe how we are now facing a similar problem in Galactic cartography as we try to reconcile older views of the Galactic disk based on the photometric distances to stars and kinematic distance to neutr作者: HIKE 時間: 2025-3-25 21:58 作者: Subjugate 時間: 2025-3-26 03:11 作者: enflame 時間: 2025-3-26 07:28
Dust in the Local Group,ects of dust extinction in inferring the true luminosity and colors of reddened astrophysical objects. Together with the extinction spectral features, the extinction curve contains important information about the dust size distribution and composition. This review summarizes our current knowledge of作者: Mosaic 時間: 2025-3-26 11:22
Milky Way Metallicities and Fossil Cosmology,of our Galaxy. In particular it is suggested that the solar vicinity provides an unrepresentative sampling of the disk MDF and that no G-dwarf problem generalizable to the whole disk can be inferred from the solar vicinity, nor constrains on the infall time scale. I suggest that the best place to lo作者: 身體萌芽 時間: 2025-3-26 15:35 作者: Cirrhosis 時間: 2025-3-26 20:47 作者: Coterminous 時間: 2025-3-26 21:21
Cloud and Star Formation in Spiral Arms,onal instabilities, arguing that the former is prevalent at lower galactic surface densities and the latter at higher. Cloud masses are also limited by stellar feedback, which can be effective before clouds reach their maximum mass. We show other properties of clouds in simulations with different le作者: 離開可分裂 時間: 2025-3-27 02:53 作者: CANON 時間: 2025-3-27 06:47 作者: Urologist 時間: 2025-3-27 12:33
Gas and Star Formation in M33: An Artistic Pathway,high resolution data to shed light on its assembly and star formation across cosmic time. I will summarize some of the key ingredients related to the formation and evolution of this galaxy, such as its dark matter, the baryonic distribution and the metallicity gradients. M33 is a pure disk galaxy wi作者: Schlemms-Canal 時間: 2025-3-27 16:12
Depicting the Early Evolution of Globular Clusters Through the Lens of Multiple Stellar Populationsout of homogeneous material. Indeed, detailed spectroscopic studies of GC long-lived low-mass stars performed with 8–10?m class telescopes, together with high-precision photometry of Galactic GCs obtained with HST, have brought compelling evidences on the presence of multiple stellar populations in 作者: Oration 時間: 2025-3-27 20:07
Globular Clusters and Two Phase Galaxy Formation: The Milky Way and Beyond,ty maps for 25 nearby early type galaxies out to, typically, 2-3?. for galaxy starlight, and 8-10?. for globular clusters. While other surveys have much larger galaxy samples, the SLUGGS “claim to fame” is its unprecedentedly wide field coverage coupled with exquisite velocity resolution (～12?km?s.)作者: 箴言 時間: 2025-3-27 23:12
Globular Clusters in the Local Group,assembly. Those hosted by galaxies in the Local Group play a key role in this work, as they may be studied in great detail on a star-by-star basis along with the surrounding field populations. In this contribution I describe how new results from the PAndAS survey are revolutionising our view of the 作者: Concrete 時間: 2025-3-28 05:35 作者: 連接 時間: 2025-3-28 09:22 作者: Eeg332 時間: 2025-3-28 10:40 作者: Ondines-curse 時間: 2025-3-28 16:25 作者: 拋棄的貨物 時間: 2025-3-28 18:49
http://image.papertrans.cn/l/image/585239.jpg作者: POWER 時間: 2025-3-28 23:58
978-3-319-37812-1Springer International Publishing Switzerland 2015作者: onlooker 時間: 2025-3-29 06:29
Lessons From the Milky Way: The Kapteyn Universe, was supported by the observation of very different mixes in stellar types in the two streams. Had Kapteyn adopted the absorption as he himself had determined it he would not have been able to arrive at a consistent picture.作者: 詞匯表 時間: 2025-3-29 10:54
,Gould’s Belt,es resulting from shell-shell collisions in the galactic plane. The origin of the Gould’s belt may be connected to instabilities in the curling gas flows downstream from the Galaxy spiral arms, forming ISM clouds and star formation complexes.作者: 顯而易見 時間: 2025-3-29 13:54
Cloud and Star Formation in Spiral Arms,ssive GMCs. We discuss in more detail interactions of clouds in the ISM, and argue that these are more complex than early ideas of cloud–cloud collisions. Finally we show ongoing work to determine whether the Milky Way is a flocculent or grand design spiral.作者: ACTIN 時間: 2025-3-29 16:59
views by the world’s leading experts in the field.Proceeding.?Our understanding of galaxy formation comes mostly from two sources: sensitive observations at high angular resolution of the high-redshift Universe, where galaxies are observed to be forming, and detailed observations of individual stars作者: 連接 時間: 2025-3-29 22:43 作者: gene-therapy 時間: 2025-3-30 00:52 作者: Haphazard 時間: 2025-3-30 08:02
The Outer Disk and Halo of Andromeda: The View with PAndAS,tensive substructure, globular clusters and a large population of dwarf galaxies. While broadly inline with our expectations of galaxy evolution in a ΛCDM universe, PAndAS has revealed an unexpected plane of co-rotating dwarf galaxies which challenges our cosmological expectations.作者: 廢止 時間: 2025-3-30 10:41 作者: Accrue 時間: 2025-3-30 14:30
Dust in the Local Group, the extinction curve contains important information about the dust size distribution and composition. This review summarizes our current knowledge of the dust extinction of the Milky Way, three Local Group galaxies (i.e., the Small and Large Magellanic Clouds, and M?31), and galaxies beyond the Local Group.作者: NADIR 時間: 2025-3-30 17:40 作者: 煞費苦心 時間: 2025-3-30 22:41
Globular Clusters in the Local Group,ng with the surrounding field populations. In this contribution I describe how new results from the PAndAS survey are revolutionising our view of the outer halo globular cluster system of Andromeda. A brief appendix provides an updated census of Local Group globular cluster systems taking into account numerous recent discoveries.作者: 極大的痛苦 時間: 2025-3-31 03:40
The Challenge of Galactic Cartography: Lessons from the Milky Way,al and molecular gas with the current and upcoming high resolution radio and infrared surveys, and multiple parallax surveys. I then provide updates on two current issues of Galactic cartography: the “stellar break” of the Milky Way and the rapid increase in the amount of data that may be used to assess models of Galactic spiral structure.作者: 有助于 時間: 2025-3-31 08:15
Conference proceedings 2015, where galaxies are observed to be forming, and detailed observations of individual stars and clouds in the Local Group, where telltale remnants from its formative time remain and similar processes operate at a low level today. The current conference focusses on key aspects of the Local Group, comp作者: 過于光澤 時間: 2025-3-31 10:05 作者: JIBE 時間: 2025-3-31 14:04 作者: Alveoli 時間: 2025-3-31 20:35 作者: 上流社會 時間: 2025-3-31 22:15 作者: 敵手 時間: 2025-4-1 01:53 作者: 討好美人 時間: 2025-4-1 08:36 作者: 證實 時間: 2025-4-1 11:44
Jan Palou?,Soňa Ehlerováerior performance in vibration suppression compared to the heuristically tuned PID controller. Moreover, the comparison between FA and AFA reveals that AFA outperforms FA in enhancing the performance of the PID controller. The PID-FA achieved a reduction percentage of up to 96.7%, while the PID-AFA 作者: Aspiration 時間: 2025-4-1 15:55 作者: 魯莽 時間: 2025-4-1 21:22
Aigen Li,Shu Wang,Jian Gao,B. W. Jiangetermined. By applying ABC method, a single unit of kitchen cabinets is predicted to cost as much as MYR 3426.32. Whereas in TDABC, the unused capacity of time and cost are ?5208.80?min and MYR ?2838.32, accordingly. It concludes that both have strengths based on industry needs, but proving TDABC’s 作者: 反感 時間: 2025-4-1 23:35
Misha Haywoodchnical requirements that AMPLE would have to satisfy, and particularly upon the requirement that the system have at least that degree of symbolic processing capability to be able to generate code for a large number manufacturing devices, which have their own native languages.作者: LATE 時間: 2025-4-2 03:50
