標題: Titlebook: Ecology of Blue Straggler Stars; Henri M. J. Boffin,Giovanni Carraro,Giacomo Beccar Book 2015 Springer-Verlag Berlin Heidelberg 2015 Blue [打印本頁] 作者: Forbidding 時間: 2025-3-21 16:07
書目名稱Ecology of Blue Straggler Stars影響因子(影響力)
書目名稱Ecology of Blue Straggler Stars影響因子(影響力)學(xué)科排名
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書目名稱Ecology of Blue Straggler Stars網(wǎng)絡(luò)公開度學(xué)科排名
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書目名稱Ecology of Blue Straggler Stars讀者反饋
書目名稱Ecology of Blue Straggler Stars讀者反饋學(xué)科排名
作者: orthopedist 時間: 2025-3-21 23:40 作者: 畏縮 時間: 2025-3-22 02:34 作者: TAG 時間: 2025-3-22 07:26 作者: 陳列 時間: 2025-3-22 11:07
https://doi.org/10.1007/978-3-319-57228-4nitial mass. In this introductory chapter, we briefly review the most important aspects concerning the evolution and nucleosynthesis of single stars, form the early stage of its formation to the final stages and death.作者: rectum 時間: 2025-3-22 16:58
Elementary Probability and Set Theory,y nebulae (CSPN). The most recent observations of cool CSPN progenitors of barium stars, as well as of carbon-rich post-common envelope systems, are providing unique constraints on the mass transfer processes.作者: rectum 時間: 2025-3-22 20:53
Wave Power and the Djursland Coast,ing a primary close to the current turn-off mass. Rather, their primaries tend to be somewhat more massive and have evolved off the main sequence, filling their Roche lobes in the past, often converting their secondaries into blue straggler stars (but more than 1 Gyr or so ago and thus they are no longer visible today as blue straggler stars).作者: cleaver 時間: 2025-3-22 21:21
Introduction to the Theory of Stellar Evolution,nitial mass. In this introductory chapter, we briefly review the most important aspects concerning the evolution and nucleosynthesis of single stars, form the early stage of its formation to the final stages and death.作者: Toxoid-Vaccines 時間: 2025-3-23 04:53 作者: strdulate 時間: 2025-3-23 06:38
Formation Channels for Blue Straggler Stars,ing a primary close to the current turn-off mass. Rather, their primaries tend to be somewhat more massive and have evolved off the main sequence, filling their Roche lobes in the past, often converting their secondaries into blue straggler stars (but more than 1 Gyr or so ago and thus they are no longer visible today as blue straggler stars).作者: 施舍 時間: 2025-3-23 11:04
Book 2015r evolution. Such stars should have exhausted their nuclear fuel and evolved long ago to become cooling white dwarfs. They are found to exist in globular clusters, open clusters, dwarf spheroidal galaxies of the Local Group, OB associations and as field stars..This book summarises the many advances 作者: 群島 時間: 2025-3-23 14:35
Blue Straggler Stars in Globular Clusters: A Powerful Tool to Probe the Internal Dynamical Evolutiousing this stellar population as probe of GC internal dynamics. In particular, the shape of the BSS radial distribution has been found to be a powerful tracer of the dynamical age of stellar systems, thus allowing the definition of the first empirical “dynamical clock”.作者: 星星 時間: 2025-3-23 19:48
Carbon-Based Polymers, Activated Carbons, not plentiful. The limitation is mostly due to the large distance to even the closest dwarf galaxies. Nevertheless, recent studies have allowed a deeper insight on the BSS photometric properties that are worth examining.作者: scoliosis 時間: 2025-3-24 01:37
Daniel N. Cassenti,Chou P. Hungng and observable astrophysical exotica. I describe some elements of the competition among stellar dynamics, stellar evolution, and other processes that control globular cluster dynamics, with particular emphasis on pathways that may lead to the formation of blue stragglers.作者: lesion 時間: 2025-3-24 04:40
https://doi.org/10.1007/978-3-662-44434-4Blue Straggler Formation; Blue Straggler Stars Overview; Dwarf Galaxies Stellar Population; Dynamical E作者: 蛛絲 時間: 2025-3-24 08:11 作者: 彎曲道理 時間: 2025-3-24 11:41 作者: MINT 時間: 2025-3-24 16:58
https://doi.org/10.1007/978-3-319-57228-4 star begins its life in the main sequence stage through the ignition of Hydrogen in its core. From here after, the life of a star is simply described as the evolution of a gaseous mass through well defined stages of equilibrium between gravitational energy and the energy produced by the nuclear rea作者: tendinitis 時間: 2025-3-24 21:08
https://doi.org/10.1007/978-3-540-71925-0e question of their origin. I review the data and ideas that were circulating from Allan Sandage’s original discovery in 1953 of “anomalous blue stars” in the globular cluster M3, up until about 1992, when what seems to have been the only previous meeting devoted to Blue Straggler Stars (BSSs) was h作者: 粘連 時間: 2025-3-25 00:02
Thermodynamic Properties of Pure Fluids,blue stragglers are characterised by: .Extensive .-body modeling of NGC 188 with empirical initial conditions reproduces the properties of the cluster, and in particular the main-sequence solar-type binary population. The current models also reproduce well the binary orbital properties of the blue s作者: 跟隨 時間: 2025-3-25 04:31
Dimensions and Properties of Piping,te of knowledge about FBSSs, drawn from an extensive literature that I searched with the aid of the ., and .. The search prior to 2000 is spotty and I make no claim of completeness. In documenting various topics I tried to use references that acknowledge important earlier investigations..Extensive .作者: 懲罰 時間: 2025-3-25 09:21
https://doi.org/10.1007/978-1-4615-0531-0GCs). The BSS specific frequency, radial distribution, chemical composition and rotational properties are presented and discussed in the framework of using this stellar population as probe of GC internal dynamics. In particular, the shape of the BSS radial distribution has been found to be a powerfu作者: 自戀 時間: 2025-3-25 15:11 作者: 主動脈 時間: 2025-3-25 17:57 作者: 被告 時間: 2025-3-25 22:19
Carlos H. Rojas-Fernandez BSc(Pharm), PharmDions overfills its Roche lobe. In this Chapter, we overview the theoretical understanding of mass transfer via Roche lobe overflow: classification, how both the donor and of the accretor respond to the mass transfer on different timescales (adiabatic response, equilibrium response, superadiabatic re作者: 太空 時間: 2025-3-26 04:10
Wave Power and the Djursland Coast,d via mass transfer within a binary. We review how computer simulations show that stellar collisions are likely to lead to relatively little mass loss and are thus effective in producing a young population of more-massive stars. The number of blue straggler stars produced by collisions will tend to 作者: 輕推 時間: 2025-3-26 05:27 作者: Facilities 時間: 2025-3-26 11:00
Best Practices of the CFD Trade,their observational predictions. These include mass transfer during binary stellar evolution—case A/B/C and D (wind Roche-lobe overflow) mass transfer, stellar collisions during single and binary encounters in dense stellar cluster, and coupled dynamical and stellar evolution of triple systems. We a作者: 馬籠頭 時間: 2025-3-26 14:14
Applied Computational Materials Modelingongoing mass transfer have all been studied in some detail. The products of stellar collisions retain memory of their parent stars and are not fully mixed. Very high initial rotation rates must be reduced by an unknown process to allow the stars to collapse to the main sequence. The more massive col作者: Lymphocyte 時間: 2025-3-26 16:51
https://doi.org/10.1007/978-3-319-30866-1ch on topics also discussed elsewhere in this book, such as the discovery and implications of bimodal radial distributions and the “double sequences” of blue stragglers that have recently been found in some clusters. However, we will focus particularly on the search for a “smoking gun” correlation b作者: 滲透 時間: 2025-3-27 00:45 作者: heterodox 時間: 2025-3-27 03:52
Ecology of Blue Straggler Stars978-3-662-44434-4Series ISSN 0067-0057 Series E-ISSN 2214-7985 作者: neutral-posture 時間: 2025-3-27 05:23 作者: Lymphocyte 時間: 2025-3-27 11:14
Henri M. J. Boffin,Giovanni Carraro,Giacomo BeccarPresents all the relevant aspects of blue straggler stars research including recent observations and theoretical models.Carefully edited extended contributions by well-known experts in blue straggler 作者: 激怒 時間: 2025-3-27 15:07 作者: 向下五度才偏 時間: 2025-3-27 19:02 作者: Flat-Feet 時間: 2025-3-27 22:32 作者: 跳脫衣舞的人 時間: 2025-3-28 04:28 作者: STALE 時間: 2025-3-28 07:27 作者: 預(yù)知 時間: 2025-3-28 14:04 作者: Firefly 時間: 2025-3-28 15:26
Blue Stragglers in Globular Clusters: Observations, Statistics and Physics, to point towards a formation channel involving binaries, rather than dynamical encounters. However, the correlation between blue straggler numbers and actual binary numbers—which relies on recently determined empirical binary fractions—is actually . than that with core mass. We explain how this sur作者: accrete 時間: 2025-3-28 19:23
Blue Stragglers in Clusters and Integrated Spectral Properties of Stellar Populations,ar evolution. Blue straggler stars (BSSs), as discussed intensively in this book both observationally and theoretically, are very important in our context when considering the integrated spectral properties of a cluster, or a simple stellar population. In this chapter, we are going to describe how i作者: fiscal 時間: 2025-3-28 23:16 作者: 易受騙 時間: 2025-3-29 03:58
Book 2015rmation channels; Dynamics of globular clusters; Interpretation of observational data and comparison with models. The book also offers an introductory chapter on stellar evolution written by the editors of the book..作者: 增長 時間: 2025-3-29 10:23 作者: 填料 時間: 2025-3-29 14:55
Dimensions and Properties of Piping,th the observations and the .-body models strongly indicate that the long-period blue-straggler binaries—which dominate the NGC 188 blue-straggler population—are formed by asymptotic-giant (primarily) and red-giant mass transfer onto main-sequence stars. The models suggest that the few non-velocity-作者: 邊緣 時間: 2025-3-29 17:35 作者: 真實的你 時間: 2025-3-29 21:44
Best Practices of the CFD Trade,d that multiple channels of BSS formation are likely to take part in producing the observed BSSs, and we point out the strengths and weaknesses of each the formation channel in respect to the observational constraints. Finally we point out directions to further explore the origin of BSS, and highlig作者: NIP 時間: 2025-3-30 01:23
Applied Computational Materials Modeling there are more possible configurations which produce blue stragglers, and there are differing contributions to the blended light of the system. The effects of rotation may be substantial in both collision and merger products, and could result in significant mixing unless angular momentum is lost sh作者: 壓倒性勝利 時間: 2025-3-30 05:49
https://doi.org/10.1007/978-3-319-30866-1 to point towards a formation channel involving binaries, rather than dynamical encounters. However, the correlation between blue straggler numbers and actual binary numbers—which relies on recently determined empirical binary fractions—is actually . than that with core mass. We explain how this sur作者: 攀登 時間: 2025-3-30 08:19
https://doi.org/10.1007/978-1-4614-1888-7ar evolution. Blue straggler stars (BSSs), as discussed intensively in this book both observationally and theoretically, are very important in our context when considering the integrated spectral properties of a cluster, or a simple stellar population. In this chapter, we are going to describe how i作者: 果核 時間: 2025-3-30 13:01
Introduction to the Theory of Stellar Evolution, star begins its life in the main sequence stage through the ignition of Hydrogen in its core. From here after, the life of a star is simply described as the evolution of a gaseous mass through well defined stages of equilibrium between gravitational energy and the energy produced by the nuclear rea作者: Arable 時間: 2025-3-30 19:09 作者: 就職 時間: 2025-3-30 23:01
The Blue Stragglers of the Old Open Cluster NGC 188,blue stragglers are characterised by: .Extensive .-body modeling of NGC 188 with empirical initial conditions reproduces the properties of the cluster, and in particular the main-sequence solar-type binary population. The current models also reproduce well the binary orbital properties of the blue s
