標(biāo)題: Titlebook: Exoplanets; Detection, Formation John W. Mason Book 2008 Springer-Verlag Berlin Heidelberg 2008 Brown Dwarfs.Evolution.Exoplanets.Extrasola [打印本頁(yè)] 作者: 熱愛 時(shí)間: 2025-3-21 17:51
書目名稱Exoplanets影響因子(影響力)
書目名稱Exoplanets影響因子(影響力)學(xué)科排名
書目名稱Exoplanets網(wǎng)絡(luò)公開度
書目名稱Exoplanets網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Exoplanets被引頻次
書目名稱Exoplanets被引頻次學(xué)科排名
書目名稱Exoplanets年度引用
書目名稱Exoplanets年度引用學(xué)科排名
書目名稱Exoplanets讀者反饋
書目名稱Exoplanets讀者反饋學(xué)科排名
作者: 鉆孔 時(shí)間: 2025-3-22 00:15 作者: Corporeal 時(shí)間: 2025-3-22 03:58 作者: Guaff豪情痛飲 時(shí)間: 2025-3-22 05:58
Formation, Dynamical Evolution, and Habitability of Planets in Binary Star Systems,iant and terrestrial planets in dual-star environments, and by presenting results of the studies of their dynamical evolution and habitability, as well as the mechanisms of delivery of water and other volatiles to their terrestrial-class objects. In this chapter, the reader is presented with a compr作者: Flat-Feet 時(shí)間: 2025-3-22 11:18 作者: 失望未來 時(shí)間: 2025-3-22 13:45
Fuzzy Multi-Objective Programming,allow measurement of planetary orbital parameters. Finally, we show that a low-cost, space-based microlensing survey can provide a comprehensive statistical census of extrasolar planetary systems with sensitivity down to 0.1 Earth-masses at separations ranging from 0.5 AU to infinity.作者: 失望未來 時(shí)間: 2025-3-22 20:05 作者: Urgency 時(shí)間: 2025-3-23 00:20
Complementary Fuzzy Incidence Graphs,ayed. With the continuous development of experiments close-orbiting terrestrial-mass extra-solar planets are the exciting new frontier in astrophysics and will test a wide range of theoretical predictions.作者: eulogize 時(shí)間: 2025-3-23 02:02 作者: Canary 時(shí)間: 2025-3-23 08:25 作者: 異端邪說下 時(shí)間: 2025-3-23 11:18
Fuzzy Filters for Noise Reduction in Images have now been discovered using other detection methods that may be more successful in detecting terrestrial-type planets. In this chapter we will review the main physical properties of the exoplanets (and their parent stars) discovered to date (28 February 2007) and will review the expectations of forthcoming observations.作者: olfction 時(shí)間: 2025-3-23 15:15 作者: 蹣跚 時(shí)間: 2025-3-23 21:30
https://doi.org/10.1007/978-1-4471-5043-5will find and study extrasolar terrestrial planets, searching for signs of life. This chapter reviews our current understanding of how we will identify planets that might support life around other stars, and incorporates results from the new science of astrobiology that support these searches作者: Iatrogenic 時(shí)間: 2025-3-23 23:53 作者: Ligament 時(shí)間: 2025-3-24 04:03 作者: aphasia 時(shí)間: 2025-3-24 07:12 作者: Alopecia-Areata 時(shí)間: 2025-3-24 12:15 作者: 令人發(fā)膩 時(shí)間: 2025-3-24 16:02 作者: 發(fā)展 時(shí)間: 2025-3-24 19:24
https://doi.org/10.1007/978-3-030-51272-9ingle-object to multi-object observations has enabled large-scale astronomical surveys (e.g., the Sloan Digital Sky Survey) and consistently led to dramatic new discoveries. We anticipate similar advances will also occur with multi-object Doppler planet surveys in the next decade.作者: 戲服 時(shí)間: 2025-3-25 02:49 作者: 空氣傳播 時(shí)間: 2025-3-25 04:42 作者: Generosity 時(shí)間: 2025-3-25 11:09
Searching for Exoplanets in the Stellar Graveyard,o be brought to bear, in some cases with much higher sensitivity, allowing the detection of low mass planets. Planets detected in the graveyard reflect the ‘live’ population of planets, and in some cases provide potentially strong constraints on planet formation processes, and the general planet population.作者: Bone-Scan 時(shí)間: 2025-3-25 15:42
978-3-642-09328-9Springer-Verlag Berlin Heidelberg 2008作者: opprobrious 時(shí)間: 2025-3-25 19:21 作者: 縮減了 時(shí)間: 2025-3-25 20:50
John W. MasonThe first collection of review articles in one volume covering the very latest developments in exoplanet research.An invaluable introduction to all the key aspects of exoplanetary systems.Contains top作者: 饑荒 時(shí)間: 2025-3-26 01:44 作者: 打折 時(shí)間: 2025-3-26 07:13 作者: 祝賀 時(shí)間: 2025-3-26 11:33
https://doi.org/10.1007/978-3-030-51272-9y single object Doppler techniques. This chapter summarizes the results of Doppler planet surveys in the past decade, and new progress and early results in the development of new Doppler techniques, especially multiple object techniques. It also presents the scientific motivation for the next genera作者: Flawless 時(shí)間: 2025-3-26 15:34 作者: 要塞 時(shí)間: 2025-3-26 16:51 作者: 新手 時(shí)間: 2025-3-26 21:45 作者: arthroplasty 時(shí)間: 2025-3-27 02:02 作者: fleeting 時(shí)間: 2025-3-27 08:10 作者: 文件夾 時(shí)間: 2025-3-27 12:32
Fuzzy Subgroups of Abelian Groups,s may remain, and in some circumstances there may be a new epoch of planet formation after the main sequence. In this chapter, scenarios for the retention and formation of planets after star death, and the prospects for detection, including current known post-main sequence systems are discussed. Pla作者: 壓碎 時(shí)間: 2025-3-27 16:11 作者: 要求比…更好 時(shí)間: 2025-3-27 18:30 作者: ascetic 時(shí)間: 2025-3-27 23:57 作者: 平靜生活 時(shí)間: 2025-3-28 02:45 作者: Orgasm 時(shí)間: 2025-3-28 10:01
Detection Methods and Properties of Known Exoplanets,alogued. The vast majority of these planets have been detected with the radial velocity technique, which is biased towards heavy, close-orbiting planets. However, the number of lighter, more distantly orbiting known exoplanets is increasing steadily and, in addition, a growing fraction of exoplanets作者: 易于交談 時(shí)間: 2025-3-28 13:17
Doppler Exoplanet Surveys: From Single Object to Multiple Objects,y single object Doppler techniques. This chapter summarizes the results of Doppler planet surveys in the past decade, and new progress and early results in the development of new Doppler techniques, especially multiple object techniques. It also presents the scientific motivation for the next genera作者: ALLAY 時(shí)間: 2025-3-28 17:34
Detection of Extrasolar Planets by Gravitational Microlensing,w-mass planets at separations of a few AU. The early evidence from microlensing indicates that the most common types of exoplanet yet detected are the so-called super-Earth planets of 10 Earth-masses at a separation of a few AU from their host stars. The detection of two such planets indicates that 作者: Glower 時(shí)間: 2025-3-28 18:59 作者: Alienated 時(shí)間: 2025-3-29 00:31
,The Brown Dwarf — Exoplanet Connection,nergy source, they cool and fade on timescales that are rapid by astronomical standards. Consequently, the observed characteristics of old, cold brown dwarfs provide insight into the expected properties of gas-giant exoplanets. This review focuses on brown dwarfs as companions to main-sequence and e作者: 驚惶 時(shí)間: 2025-3-29 05:52 作者: Kidney-Failure 時(shí)間: 2025-3-29 09:27
Dynamics of Multiple Planet Systems,(long-term) effects. Basic analytical and numerical techniques can describe these interactions. Multiple planet systems may also evolve chaotically, and some principles of chaos theory are described. Finally, this chapter discusses the current distributions of dynamical properties of exoplanetary sy作者: 材料等 時(shí)間: 2025-3-29 11:41
