標(biāo)題: Titlebook: Astrophysics in the Next Decade; The James Webb Space Harley A. Thronson,Massimo Stiavelli,Alexander Tie Conference proceedings 2009 Spring [打印本頁] 作者: 萬靈藥 時間: 2025-3-21 19:21
書目名稱Astrophysics in the Next Decade影響因子(影響力)
書目名稱Astrophysics in the Next Decade影響因子(影響力)學(xué)科排名
書目名稱Astrophysics in the Next Decade網(wǎng)絡(luò)公開度
書目名稱Astrophysics in the Next Decade網(wǎng)絡(luò)公開度學(xué)科排名
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書目名稱Astrophysics in the Next Decade被引頻次學(xué)科排名
書目名稱Astrophysics in the Next Decade年度引用
書目名稱Astrophysics in the Next Decade年度引用學(xué)科排名
書目名稱Astrophysics in the Next Decade讀者反饋
書目名稱Astrophysics in the Next Decade讀者反饋學(xué)科排名
作者: 叢林 時間: 2025-3-21 23:58 作者: Etymology 時間: 2025-3-22 04:16 作者: 脆弱么 時間: 2025-3-22 07:14 作者: 哄騙 時間: 2025-3-22 11:22
Working with Data in Flex Applicationsng motivated by a rapidly growing body of theoretical work. Numerical simulations of reionization are starting to achieve the dynamical range required to resolve galactic sources across the scale of hundreds of comoving Mpc, larger than the biggest ionized regions.作者: 宴會 時間: 2025-3-22 13:08
The Future of Ultracool Dwarf Science with JWST,low mass objects in clusters and nearby cold dwarfs from the disk population, will be seen for the first time. In combination with other groundand space-based assets and programs, JWST will usher in a new golden era of brown dwarf science and discovery.作者: occurrence 時間: 2025-3-22 20:43
Transiting Exoplanets with JWST, require tens to hundreds of hours of . time per planet. We review what is known about the physical characteristics of transiting planets, summarize lessons learned from . high-contrast exoplanet measurements, and give several examples of potential . observations.作者: 旁觀者 時間: 2025-3-22 23:44
The Frontier of Reionization: Theory and Forthcoming Observations,ng motivated by a rapidly growing body of theoretical work. Numerical simulations of reionization are starting to achieve the dynamical range required to resolve galactic sources across the scale of hundreds of comoving Mpc, larger than the biggest ionized regions.作者: 聲明 時間: 2025-3-23 03:12 作者: 薄荷醇 時間: 2025-3-23 06:37
Flex with Photoshop and Illustrator,d radiative feedback into molecular clouds—that are critical to our understanding of the formation and survival of large star clusters, topics that will be the drivers of the observations of the next decade.作者: insecticide 時間: 2025-3-23 10:34
Livecycle Data Services Case Studythe observational techniques used to discover and characterize the phases of baryons. In the spirit of the meeting, the level is aimed at a diverse and non-expert audience and additional attention is given to describe how space missions expected to launch within the next decade will impact this scientific field.作者: 協(xié)議 時間: 2025-3-23 16:16 作者: 壯觀的游行 時間: 2025-3-23 18:56 作者: 開頭 時間: 2025-3-24 00:26
Conference proceedings 2009he most challenging questions in astronomy. Although motivated and designed to study the very early Universe, the performance of the observatory’s instruments over a very wide wavelength range will allow the world’s scientific community unequaled ability to study cosmic phenomena as diverse as small作者: oracle 時間: 2025-3-24 05:41
Flex Video Gallery with Drag-and-Drop,avelengths, concepts that would later be regarded as politically unrealistic given the costs associated with them. We also explore how the fortunes of the planned Next Generation Space Telescope were intimately linked to that of its “parent,” the Hubble Space Telescope.作者: CHASE 時間: 2025-3-24 09:08
https://doi.org/10.1007/978-1-4302-0444-2in the early universe and their local counterparts; the detailed stellar populations of distant galaxies while the bulk of their stellar mass is being formed; the structure and dynamics of galaxies as they settle onto the Hubble sequence; and the physics of “feedback”, a crucial, yet poorly understood ingredient in models of galaxy formation.作者: CAMEO 時間: 2025-3-24 11:25
Beyond the Hubble Space Telescope: Early Development of the Next Generation Space Telescope,avelengths, concepts that would later be regarded as politically unrealistic given the costs associated with them. We also explore how the fortunes of the planned Next Generation Space Telescope were intimately linked to that of its “parent,” the Hubble Space Telescope.作者: 商議 時間: 2025-3-24 15:46 作者: Engaging 時間: 2025-3-24 21:07 作者: 鍵琴 時間: 2025-3-25 01:12
Introducing Flex and Flex Builder 3,. In particular, I discuss what is known about the stellar IMF and the nature of dense cores on the verge of star formation. I then discuss how these two topics contribute to our general understanding of the origin of stellar mass, the key mystery in the star formation process.作者: 不感興趣 時間: 2025-3-25 06:10 作者: 撫育 時間: 2025-3-25 10:10
Astrophysics and Space Science Proceedingshttp://image.papertrans.cn/b/image/163702.jpg作者: 混合,攙雜 時間: 2025-3-25 12:21 作者: Acquired 時間: 2025-3-25 16:48
Flex Video Gallery with Drag-and-Drop,ce Telescope. We argue that the initial ideas for such a Next Generation Space Telescope were developed in the context of the planning for a successor to the Hubble Space Telescope. Much the most important group of astronomers and engineers examining such a successor was based at the Space Telescope作者: ALT 時間: 2025-3-25 22:37 作者: Impugn 時間: 2025-3-26 00:14 作者: 小母馬 時間: 2025-3-26 04:37 作者: Intervention 時間: 2025-3-26 11:09
Introducing Flex and Flex Builder 3,plex one and its solution depends critically on empirical data. In this contribution, I review some of the progress that has been achieved in identifying and measuring the fundamental boundary and initial conditions that constrain the solution and must be met by any complete theory of star formation作者: GENUS 時間: 2025-3-26 16:21 作者: Inferior 時間: 2025-3-26 20:46 作者: nitric-oxide 時間: 2025-3-26 21:28
Flex with Photoshop and Illustrator,ng of the star formation process in starbursts and super star clusters—initial mass functions, cluster mass functions, star formation efficiencies, and radiative feedback into molecular clouds—that are critical to our understanding of the formation and survival of large star clusters, topics that wi作者: Substance 時間: 2025-3-27 01:34 作者: 使?jié)M足 時間: 2025-3-27 08:58 作者: chronology 時間: 2025-3-27 13:13
https://doi.org/10.1007/978-1-4302-0444-2ound us today. The redshift range, 1.5 ? z ? 3.5 represents a crucial epoch for observing the assembly of the modern galaxy population, which is largely in place by z ～ 1. There has been tremendous progress assembling observations at z>1.5 over the past decade. Yet, many challenges remain. The next 作者: 滴注 時間: 2025-3-27 15:31 作者: 偽造者 時間: 2025-3-27 20:04
Interacting with the Web Browser formation and the reionization process. Although its evolution may seem straightforward, a number of feedback mechanisms can dramatically affect it. Radiative feedback, through a Lyman-Werner background, an X-ray background, and photoionization, affect halo collapse and the clumping of the IGM. We 作者: auxiliary 時間: 2025-3-28 01:40
Working with Data in Flex Applications. M., and low-mass black holes (BHs), with a mass of several $× 10. M. should be directly detectable out to redshift z = 10, and individual supernovae (SNe) and gamma ray burst GRB afterglows are bright enough to be visible beyond this redshift. Dense primordial gas, in the process of collapsing fro作者: Armada 時間: 2025-3-28 03:59
Livecycle Data Services Case Study Our summary examines on three milestone redshifts since the reionization of H in the IGM, z = 3, 1, and 0, with emphasis on the endpoints. We review the observational techniques used to discover and characterize the phases of baryons. In the spirit of the meeting, the level is aimed at a diverse an作者: Seizure 時間: 2025-3-28 09:11 作者: 爵士樂 時間: 2025-3-28 12:35 作者: 受人支配 時間: 2025-3-28 15:01 作者: Psa617 時間: 2025-3-28 21:39
Flex with Photoshop and Illustrator,will discuss the main options for using JWST and concurrent facilities to study the early, gas-rich, massive phases of protoplanetary disks. We discuss the opportunities to study gas and dust in such disks and to derive constraints on physical and chemical processes taking place there.作者: 使熄滅 時間: 2025-3-29 00:14
https://doi.org/10.1007/978-1-4020-9457-6Accretion; Exoplanet discovery; Galaxy Evolution; Hubble successor; JWST; James Webb Space Telescope; Reds作者: Exposition 時間: 2025-3-29 06:38
978-90-481-8132-2Springer Science+Business Media B.V. 2009作者: zonules 時間: 2025-3-29 10:32
Accretion Disks Before (?) the Main Planet Formation Phase,will discuss the main options for using JWST and concurrent facilities to study the early, gas-rich, massive phases of protoplanetary disks. We discuss the opportunities to study gas and dust in such disks and to derive constraints on physical and chemical processes taking place there.作者: Figate 時間: 2025-3-29 12:22 作者: 彎彎曲曲 時間: 2025-3-29 19:21
Flex Video Gallery with Drag-and-Drop,nsitivity of ALMA, Herschel, SOFIA, JWST and ELTs across the full range of wavelengths from cm to μm will be essential to trace this lifecycle of gas and dust from clouds to planets. The continued need for basic molecular data on gaseous and solid-state material coupled with powerful radiative trans作者: cogitate 時間: 2025-3-29 20:41 作者: 寬敞 時間: 2025-3-30 00:44 作者: MODE 時間: 2025-3-30 07:18 作者: Deceit 時間: 2025-3-30 09:16 作者: 輕打 時間: 2025-3-30 13:45 作者: 相符 時間: 2025-3-30 18:53 作者: 噴出 時間: 2025-3-30 22:24 作者: 初次登臺 時間: 2025-3-31 04:53 作者: 拱墻 時間: 2025-3-31 06:29
Astrochemistry of Dense Protostellar and Protoplanetary Environments,nsitivity of ALMA, Herschel, SOFIA, JWST and ELTs across the full range of wavelengths from cm to μm will be essential to trace this lifecycle of gas and dust from clouds to planets. The continued need for basic molecular data on gaseous and solid-state material coupled with powerful radiative trans作者: CULP 時間: 2025-3-31 09:47
Prospects for Studies of Stellar Evolution and Stellar Death in the , Era,ey water-ice and crystalline silicate bands. . has significantly increased the number of Type II supernovae that have been surveyed for early-epoch dust formation but reliable quantification of the dust contributions from massive star supernovae of Type II, Type Ib and Type Ic to low- and high-redsh作者: 油膏 時間: 2025-3-31 16:08 作者: 招惹 時間: 2025-3-31 19:55 作者: defile 時間: 2025-4-1 00:52 作者: 有節(jié)制 時間: 2025-4-1 04:09
Observing the First Stars and Black Holes,lar clusters and intermediate-mass black holes at z > 10 will likely fall below .’s detection threshold. However, . could reveal a decline at the faint-end of the high-redshift luminosity function, and thereby shed light on radiative and other feedback effects that operate at these early epochs. . w
