標(biāo)題: Titlebook: Stellar Astrophysics; A Tribute to Helmut K. S. Cheng,K. C. Leung,T. P. Li Conference proceedings 2003 Springer Science+Business Media Dor [打印本頁] 作者: Jejunum 時間: 2025-3-21 17:52
書目名稱Stellar Astrophysics影響因子(影響力)
書目名稱Stellar Astrophysics影響因子(影響力)學(xué)科排名
書目名稱Stellar Astrophysics網(wǎng)絡(luò)公開度
書目名稱Stellar Astrophysics網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Stellar Astrophysics被引頻次
書目名稱Stellar Astrophysics被引頻次學(xué)科排名
書目名稱Stellar Astrophysics年度引用
書目名稱Stellar Astrophysics年度引用學(xué)科排名
書目名稱Stellar Astrophysics讀者反饋
書目名稱Stellar Astrophysics讀者反饋學(xué)科排名
作者: 學(xué)術(shù)討論會 時間: 2025-3-21 20:19
Gamma-Ray Pulsars in Gould Belt and Unidentified Gamma-Ray Sources in Medium Latitudes can exist even their age > 10. yr old. We use Monte Carlo techniques to simulate the statistical properties of rotation-powered pulsars in the Gould Belt. If the pulsar birth rate in Gould Belt is 3 × 10..., the gamma-ray pulsars in this region, which can be detected by EGRET, will must be dominate作者: misanthrope 時間: 2025-3-22 01:55
Magnetars and Pulsars: A Missing Link fields, i.e., magnetars, marking them a distinguished species from the conventional species of spindown-powered isolated neutron stars, i.e., radio pulsars. The current arguments in favor of the magnetar interpretation of SGR/AXP phenomenology will be outlined, and the two energy sources in magneta作者: 西瓜 時間: 2025-3-22 05:07 作者: 流利圓滑 時間: 2025-3-22 09:35 作者: 假裝是我 時間: 2025-3-22 13:59 作者: Inflated 時間: 2025-3-22 18:11 作者: PURG 時間: 2025-3-23 00:16
Phase Transition in Rotating Hybrid Starsmoment of inertia, and even results in an era of spin-up of the pulsar (Glendenning, Pei, & Weber 1997, hereafter GPW) . We have found that the equation of states of the crust of neutron star and the accuracy of the numerical models which can be used to determinate the stellar rotating properties ar作者: Lipohypertrophy 時間: 2025-3-23 03:06
Accretion Disk Oscillations and QPOs in X-Ray Binariesation modes in a relativistic accretion disk. Here we studied the non-damping feature of some oscillation modes by considering the radial perturbations and viscosity effects. We found that the non-damping fundamental modes can be amplified significantly in the inner disk when the viscosity parameter作者: charisma 時間: 2025-3-23 09:29
Bare Strange Quark Stars: Formation and Emissionmperature after the supernova detonation flame, and a crust can also hardly form except for a super-Eddington accretion. The magnetosphere of a bare strange star is composed mainly of e. pair plasma, where both inner and outer vacuum gaps work for radio as well as high energy nonthermal emission. A 作者: ADAGE 時間: 2025-3-23 10:25 作者: 無思維能力 時間: 2025-3-23 14:37 作者: Distribution 時間: 2025-3-23 20:19 作者: 痛恨 時間: 2025-3-24 01:57
Case B Binary Evolution Compared to Observed Algolsns were done with and without the assumption of conservative mass transfer, giving very different results for the distributions of mass ratios and orbital periods for the obtained Algols. The conservative model fits the observations poorly by producing far too many Algols with low mass ratios and la作者: 全部逛商店 時間: 2025-3-24 03:51 作者: 雪上輕舟飛過 時間: 2025-3-24 08:59
Gamma-Ray Pulsars in Gould Belt and Unidentified Gamma-Ray Sources in Medium LatitudesBelt. If the pulsar birth rate in Gould Belt is 3 × 10..., the gamma-ray pulsars in this region, which can be detected by EGRET, will must be dominated by those pulsars with large inclination angles. We predict that these gamma-ray pulsars should have a wider period P~ (0.5–0.8)s and with a typical age of several million years old.作者: 招惹 時間: 2025-3-24 13:24
Beaming Effects in Gamma-Ray Burstsivistic phase, which typically occurs at time 10 to 30 days. The break is affected by many parameters, especially by the electron energy fraction (&), and the magnetic energy fraction (math). Implication of orphan afterglow surveys on GRB beaming is investigated. The possible existence of a kind of cylindrical jets is also discussed.作者: 親愛 時間: 2025-3-24 15:24 作者: Antecedent 時間: 2025-3-24 20:08
Properties of Cloudy Bag Strange Starsfining bag is introduced such that Chiral symmetry is conserved. The temperature evolution can provide a possible way to distinguish a compact object between a neutron star, MIT strange star and Cloudy Bag strange star in observations.作者: Herd-Immunity 時間: 2025-3-24 23:41 作者: 倒轉(zhuǎn) 時間: 2025-3-25 04:05 作者: invulnerable 時間: 2025-3-25 11:14
Bare Strange Quark Stars: Formation and Emissionfeatureless thermal spectrum is expected since no ion is above the quark surface, whilst electron cyclotron lines could appear in some bare strange stars with suitable magnetic fields. Various astrophysical implications of bare strange stars are discussed.作者: 軍火 時間: 2025-3-25 12:39
Wide Binaries in the Orion Nebula Clustersample with a high expectation of them being physical systems. We have identified 68 such pairs of stars with projected separations between 2000 and 33 000 astronomical units. The distribution of separations . seems to be Oepik-like, i.e. ..作者: 壓倒性勝利 時間: 2025-3-25 19:11
Case B Binary Evolution Compared to Observed Algolsrge orbital periods. Liberal models yield better agreement between theory and observations. The best agreement is obtained when ≈ 50% of the mass lost by the primary is trapped into a ring with radius ≈2.5 × the semi major axis of the binary orbit.作者: 感情脆弱 時間: 2025-3-25 21:43 作者: 很像弓] 時間: 2025-3-26 02:38
GRB Opening Angle & Space Density Distribution Determined from the GRB Intensity Distribution11.7, suggesting that either the actual star formation rate should peak at significantly higher z than believed previously, or GRBs do not follow the star formation rate for z > 1. The existence of the lower-bound z = 0.28 ± 0.04 for GRB production indicates absence or a much lower rate of massive star formation at the present time.作者: Spina-Bifida 時間: 2025-3-26 08:11
Accretion Disk Oscillations and QPOs in X-Ray Binarieshe spin of the central object. Some observed properties of kilohertz QPOs in neutron star X-ray binaries and hundred-hertz QPOs in black hole X-ray binaries may be explained by these trapped non-damping oscillation modes.作者: Bravado 時間: 2025-3-26 08:53 作者: oxidant 時間: 2025-3-26 16:20
aim is to illustrate an ‘a(chǎn)esthetic move’ in social sciences and in particular in health and in education. The collection builds a bridge between the Arts and Health and Education by offering innovative exemplars of use of poetry in social science research and in the context of the many varied disci作者: languor 時間: 2025-3-26 17:54
T. Lu aim is to illustrate an ‘a(chǎn)esthetic move’ in social sciences and in particular in health and in education. The collection builds a bridge between the Arts and Health and Education by offering innovative exemplars of use of poetry in social science research and in the context of the many varied disci作者: FEIGN 時間: 2025-3-26 23:55
T. P. Lie, beyond academia, and offers a challenge to conventional qThis volume offers a novel collection of international works on the use of poetry in inquiry that transcends conventional disciplinary boundaries. The aim is to illustrate an ‘a(chǎn)esthetic move’ in social sciences and in particular in health a作者: 不愿 時間: 2025-3-27 02:55 作者: 夜晚 時間: 2025-3-27 05:42 作者: transdermal 時間: 2025-3-27 09:33 作者: 相符 時間: 2025-3-27 16:31
Y. F. Huang,T. Lu,Z. G. Dai,K. S. ChengR. Curtius besch?ftigte diese Frage sehr. Eine endgültige Antwort hat er darauf leider 1 nicht mehr geben k?nnen ? Die Zusammenstellung der europ?ischen Poetiken 2 von Saintsbury und Spingarn bewies offensichtlich die Unwirksamkeit des Aristotelismus in der spanischen Literatur des 16. und 17. Jahrh作者: 欺騙手段 時間: 2025-3-27 21:14
J. R. Lin,S. N. Zhang,T. P. Li give poetry its cultural identity.Poetics of Curriculum, PoThrough multiple lenses of curriculum studies, the author explores how poetry is situated in the pedagogical world. Her work aims to illuminate how poetry is studied in schools and how these practices of studying poetry give poetry its cult作者: 抓住他投降 時間: 2025-3-28 00:02
J. Hu,S. N. Zhang,T. P. Lietry is studied in schools and how these practices of studying poetry give poetry its cultural identity. Each chapter is guided by insight from John Dewey’s Art as Experience which promotes explorations of opportunities for students to have profound experiences with poetry and art in schools. The pu作者: 侵略 時間: 2025-3-28 04:08 作者: 消滅 時間: 2025-3-28 09:38 作者: 使增至最大 時間: 2025-3-28 14:20 作者: Repetitions 時間: 2025-3-28 16:34
C. Y. Ng,K. S. Cheng,M. C. Chu give poetry its cultural identity.Poetics of Curriculum, PoThrough multiple lenses of curriculum studies, the author explores how poetry is situated in the pedagogical world. Her work aims to illuminate how poetry is studied in schools and how these practices of studying poetry give poetry its cult作者: nutrients 時間: 2025-3-28 20:19 作者: GRIPE 時間: 2025-3-29 01:06 作者: 干旱 時間: 2025-3-29 05:16
Dany Vanbeveren,Erwin De Donderome aspects of this activity may help to define the kinds of poetry which are the focus of the other essays here. A small press is one, or rarely more than two individuals who, usually in their spare time and at their own expense, write or edit poetry, print and bind it more or less competently, and作者: negligence 時間: 2025-3-29 07:58 作者: hyperuricemia 時間: 2025-3-29 11:54 作者: 埋伏 時間: 2025-3-29 18:15 作者: 明智的人 時間: 2025-3-29 22:32
Timescale Spectra in High Energy Astrophysicsabilities of hard X-rays from neutron star and black hole binaries, γ-ray bursts and terrestrial γ-ray flashes. The results indicate that the time domain method of spectral analysis is a powerful tool in revealing the underlying physics in high-energy processes in objects.作者: 灌輸 時間: 2025-3-30 01:24 作者: nitric-oxide 時間: 2025-3-30 06:48 作者: 有其法作用 時間: 2025-3-30 10:33 作者: 高度 時間: 2025-3-30 15:45
Very Cool Close Binary SystemsWith the advent of modern surveys which yield more M-type eclipsing binary stars and with a new light curve analysis code which incorporates atmospheric models for cool stars, the time is right for a renaissance in understanding the lower main sequence.作者: 填滿 時間: 2025-3-30 19:18 作者: 主動 時間: 2025-3-30 23:06 作者: 哀悼 時間: 2025-3-31 03:04 作者: 疾馳 時間: 2025-3-31 05:27
978-90-481-6452-3Springer Science+Business Media Dordrecht 2003作者: 箴言 時間: 2025-3-31 11:14
Stellar Astrophysics978-94-017-0403-8Series ISSN 0067-0057 Series E-ISSN 2214-7985 作者: 中子 時間: 2025-3-31 13:41
Conference proceedings 2003the Local Organizing Committee. Initially, Professor Lu was the logical choice but he declined for personal reasons. Professor Li was invited to lead a new department of Astrophysics at Tsinghua University so he could not take on the additional load of chairing the LOC. Professor Gang Zhao of Beijin
