標(biāo)題: Titlebook: Double Stars, Physical Properties and Generic Relations; Proceeding of IAU Co Bambang Hidayat,Zdeněk Kopal,Jürgen Rahe Conference proceedin [打印本頁(yè)] 作者: 小缺點(diǎn) 時(shí)間: 2025-3-21 18:42
書目名稱Double Stars, Physical Properties and Generic Relations影響因子(影響力)
書目名稱Double Stars, Physical Properties and Generic Relations影響因子(影響力)學(xué)科排名
書目名稱Double Stars, Physical Properties and Generic Relations網(wǎng)絡(luò)公開度
書目名稱Double Stars, Physical Properties and Generic Relations網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Double Stars, Physical Properties and Generic Relations被引頻次
書目名稱Double Stars, Physical Properties and Generic Relations被引頻次學(xué)科排名
書目名稱Double Stars, Physical Properties and Generic Relations年度引用
書目名稱Double Stars, Physical Properties and Generic Relations年度引用學(xué)科排名
書目名稱Double Stars, Physical Properties and Generic Relations讀者反饋
書目名稱Double Stars, Physical Properties and Generic Relations讀者反饋學(xué)科排名
作者: 壓迫 時(shí)間: 2025-3-21 20:39 作者: Sedative 時(shí)間: 2025-3-22 01:56 作者: NEX 時(shí)間: 2025-3-22 06:54 作者: 伸展 時(shí)間: 2025-3-22 10:09 作者: erythema 時(shí)間: 2025-3-22 16:10
https://doi.org/10.1007/978-981-15-5366-0star census for all kind of systems: close, medium, and wide. The Hipparcos satellite will probably add some important informations in that respect but ground-based observations also remain of the highest importance (radial velocities, photometry, astrometry, etc.).作者: erythema 時(shí)間: 2025-3-22 20:01 作者: Ophthalmoscope 時(shí)間: 2025-3-22 21:26
Madhumita Bandyopadhyay,Sunita Chughe speckle interferometric measurements of a sufficiently large sample of close visual binaries are suggested to settle this important observational question. The present paper is special in that it brings together a wealth of useful information, both observational and theoretical, in one place.作者: 乞討 時(shí)間: 2025-3-23 03:53
Sandeep Narula,Narma Bhattacharyartance, because it is only one of very few earlytype systems for which reliable limb-darkening coefficients can be expected to be obtained. The contribution of the light of the third component to the system has also been determined, and it appears most likely that VV Ori C is a star of spectral type A3 V.作者: 障礙 時(shí)間: 2025-3-23 06:55 作者: curriculum 時(shí)間: 2025-3-23 10:51
Duplicity on the Main Sequence,pay special attention to nearby binary stars. On the other hand, we do not have the space to discuss in any detail the binaries in extragalactic systems, in the upper regions of the HR-diagram; they are practically all evolved systems.作者: expeditious 時(shí)間: 2025-3-23 16:43
Binary Statistics and Star Formation,e speckle interferometric measurements of a sufficiently large sample of close visual binaries are suggested to settle this important observational question. The present paper is special in that it brings together a wealth of useful information, both observational and theoretical, in one place.作者: projectile 時(shí)間: 2025-3-23 20:05 作者: 充滿人 時(shí)間: 2025-3-23 22:44 作者: 新陳代謝 時(shí)間: 2025-3-24 05:53 作者: 稀釋前 時(shí)間: 2025-3-24 09:21 作者: RECUR 時(shí)間: 2025-3-24 13:06
Samuel Alexander,Brendan Gleesonough a Laval-nozzle-effect at the inner Lagrangian point of the system and powering of the emission lines through kinetic energy losses of Coriolis deflected and subsequently colliding gas streams are considered as possible mechanisms at work in the system.作者: 被告 時(shí)間: 2025-3-24 15:17 作者: 輕信 時(shí)間: 2025-3-24 19:53
https://doi.org/10.1007/978-94-009-6372-6Galaxy; Variation; astronomy; galaxies; star; star formation; stellar; stellar evolution作者: 開始發(fā)作 時(shí)間: 2025-3-24 23:35
978-94-009-6374-0D. Reidel Publishing Company, Dordrecht, Holland 1984作者: Additive 時(shí)間: 2025-3-25 04:59 作者: Dictation 時(shí)間: 2025-3-25 08:42
https://doi.org/10.1007/978-981-15-5366-0, our beloved colleague Vainu Bappu — past President of the International Astronomical Union, and life-long student of the subject of our Colloquium — is no longer in this world to take his rightful place among us; and, therefore, my remarks which follow can be dedicated only to his memory.作者: 怕失去錢 時(shí)間: 2025-3-25 13:28 作者: 滔滔不絕地說(shuō) 時(shí)間: 2025-3-25 17:17 作者: 盡管 時(shí)間: 2025-3-25 23:01 作者: 內(nèi)向者 時(shí)間: 2025-3-26 02:22 作者: 樂(lè)章 時(shí)間: 2025-3-26 07:44 作者: FLACK 時(shí)間: 2025-3-26 11:29
Daniel Zünd,Luís M. A. Bettencourt available on the spectral variations at optical wavelengths these stars undergo. I do not give extensive references to those data, for previous reviews have done so quite adequately. Rather, I concentrate on the extensive widening of the wavebands within which symbiotic stars have been studied over作者: hangdog 時(shí)間: 2025-3-26 16:00 作者: Fretful 時(shí)間: 2025-3-26 18:37 作者: 欺騙世家 時(shí)間: 2025-3-26 21:40
Sandeep Narula,Narma Bhattacharyamponent whose orbital period about the eclipsing pair is about 120 days. In recent years there have been several new photoelectric and spectroscopic investigations of this system, and the results of these are compared. Both the geometric and photometric orbital elements appear to be well determined.作者: CHECK 時(shí)間: 2025-3-27 02:58
https://doi.org/10.1007/978-981-16-4888-54.In order to assess the relative importance of massive binary evolution as one of the ways to produce WR stars, the galactic distribution of WR binaries is compared with that of single WR stars using improved intrinsic parameters and new data for the fainter WR stars..In the galactic plane the incr作者: PIZZA 時(shí)間: 2025-3-27 07:23 作者: habile 時(shí)間: 2025-3-27 10:23 作者: COM 時(shí)間: 2025-3-27 17:38 作者: 圖表證明 時(shí)間: 2025-3-27 19:02 作者: Notify 時(shí)間: 2025-3-27 23:50
https://doi.org/10.1007/978-981-16-0893-3The photometric variability of CPD-48.1577 in the optical and IR ranges is discussed. The structure and variation of prominent emission line profiles are investigated. An estimate of the distance is given.作者: Dri727 時(shí)間: 2025-3-28 05:43 作者: AVOW 時(shí)間: 2025-3-28 06:55 作者: Ganglion-Cyst 時(shí)間: 2025-3-28 12:14
Fission Sequence and Equilibrium Models of Rigidity Rotating Polytropes,Equilibrium sequences of self-gravitating and polytropic stars including binary stars are computed for various polytropic indexes. We find a fission sequence from an ellipsoidal configuration to a binary by way of dumb-bell equilibrium.作者: 謙虛的人 時(shí)間: 2025-3-28 15:22 作者: 確定的事 時(shí)間: 2025-3-28 19:33
A Catalogue and Finding List of Galactic Novae,A catalogue of galactic novae and an atlas of finding charts are under preparation and will be published in 1984. The status of the project is described.作者: MUTE 時(shí)間: 2025-3-29 02:50 作者: 敏捷 時(shí)間: 2025-3-29 04:36
,Spectroscopy and Optical/IR Photometry of the Cataclysmic Variable CPD -48°1577,The photometric variability of CPD-48.1577 in the optical and IR ranges is discussed. The structure and variation of prominent emission line profiles are investigated. An estimate of the distance is given.作者: EWE 時(shí)間: 2025-3-29 10:57 作者: 手銬 時(shí)間: 2025-3-29 14:47 作者: 分開 時(shí)間: 2025-3-29 16:11
http://image.papertrans.cn/e/image/282691.jpg作者: 骨 時(shí)間: 2025-3-29 20:23
Evolution of Binary Systems and Their Generic Relations,, our beloved colleague Vainu Bappu — past President of the International Astronomical Union, and life-long student of the subject of our Colloquium — is no longer in this world to take his rightful place among us; and, therefore, my remarks which follow can be dedicated only to his memory.作者: 商談 時(shí)間: 2025-3-30 00:46 作者: 偽造者 時(shí)間: 2025-3-30 06:55
The Old Nova BT Monocerotis,ough a Laval-nozzle-effect at the inner Lagrangian point of the system and powering of the emission lines through kinetic energy losses of Coriolis deflected and subsequently colliding gas streams are considered as possible mechanisms at work in the system.作者: 并入 時(shí)間: 2025-3-30 09:55 作者: exigent 時(shí)間: 2025-3-30 12:39 作者: dowagers-hump 時(shí)間: 2025-3-30 18:10 作者: nonsensical 時(shí)間: 2025-3-30 23:07
The Importance of Wide-System Studies for Stellar Evolution and Galactic Dynamics,e visual pairs (short periods) may lead to mass-determinations in a relatively short time interval. But mass-determination should not be considered as the only interest of double star astronomy, even if it is of a fundamental nature..Today, it appears that researches on the origin and the evolution 作者: 吝嗇性 時(shí)間: 2025-3-31 01:50 作者: Inflated 時(shí)間: 2025-3-31 07:27 作者: Resistance 時(shí)間: 2025-3-31 11:36 作者: Bph773 時(shí)間: 2025-3-31 14:42 作者: Axillary 時(shí)間: 2025-3-31 21:27
Symbiotic Stars, available on the spectral variations at optical wavelengths these stars undergo. I do not give extensive references to those data, for previous reviews have done so quite adequately. Rather, I concentrate on the extensive widening of the wavebands within which symbiotic stars have been studied over作者: Condescending 時(shí)間: 2025-3-31 22:27
,Radial Velocity and Profile Variations of the Ultraviolet Circumstellar Lines in ζ Tauri,l atoms, and once or twice-ionized ions (except CII, Al III, Si III resonance lines) follow the same velocity variations as in the visual spectra, while the Si IV and C IV resonance lines show a constant negative velocity (～ —50 km s. at the core). The Al III, C II resonance lines and probably Fe II作者: 神刊 時(shí)間: 2025-4-1 02:04 作者: Malcontent 時(shí)間: 2025-4-1 08:16
VV Orionis: A Well-Behaved Early-Type Eclipsing Binary System,mponent whose orbital period about the eclipsing pair is about 120 days. In recent years there have been several new photoelectric and spectroscopic investigations of this system, and the results of these are compared. Both the geometric and photometric orbital elements appear to be well determined.作者: Delirium 時(shí)間: 2025-4-1 10:21
Wolf-Rayet Binaries: Evolutionary Causes for their Distribution in the Galaxy,4.In order to assess the relative importance of massive binary evolution as one of the ways to produce WR stars, the galactic distribution of WR binaries is compared with that of single WR stars using improved intrinsic parameters and new data for the fainter WR stars..In the galactic plane the incr
