標(biāo)題: Titlebook: Light on Dark Matter; Proceedings of the F Frank P. Israel Conference proceedings 1986 D. Reidel Publishing Company, Dordrecht, Holland 198 [打印本頁] 作者: incontestable 時(shí)間: 2025-3-21 18:03
書目名稱Light on Dark Matter影響因子(影響力)
書目名稱Light on Dark Matter影響因子(影響力)學(xué)科排名
書目名稱Light on Dark Matter網(wǎng)絡(luò)公開度
書目名稱Light on Dark Matter網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Light on Dark Matter被引頻次
書目名稱Light on Dark Matter被引頻次學(xué)科排名
書目名稱Light on Dark Matter年度引用
書目名稱Light on Dark Matter年度引用學(xué)科排名
書目名稱Light on Dark Matter讀者反饋
書目名稱Light on Dark Matter讀者反饋學(xué)科排名
作者: recede 時(shí)間: 2025-3-21 20:13
Heliocentric Dependences of Zodiacal Emission, Temperature and Albedomodel-dependence is reduced, compared to the values averaged on the line-of-sight. The temperature probably does not exceed 250 K at the distance of the Earth. The albedo is found to decrease from ~ 0.08 at the distance of the Earth to ~ 0.06 at the distance of Mars.作者: Blazon 時(shí)間: 2025-3-22 00:49 作者: 性冷淡 時(shí)間: 2025-3-22 08:36
IRAS Intrinsic Colours of Hot Starscz (1979) models from the visual to 12 μm results in a 12 μm flux that is about 10 percent too low, and b) The energy distribution for hot stars from 0.4 to 12 μm cannot be described with a one-temperature blackbody.作者: bronchodilator 時(shí)間: 2025-3-22 09:58
The Disc Structure and Mass Loss Rates of Be Starsree-free radiation from the disc. The density structures of the discs suggest that matter is accelerated outwards. The mass loss rates are of the order 7 10. to 2 10. M./yr, i.e. a factor 100 larger than derived from UV resonance lines (Snow, 1981).作者: nullify 時(shí)間: 2025-3-22 15:22 作者: blister 時(shí)間: 2025-3-22 19:08 作者: extinguish 時(shí)間: 2025-3-22 23:33 作者: Hirsutism 時(shí)間: 2025-3-23 01:41 作者: slow-wave-sleep 時(shí)間: 2025-3-23 07:44 作者: 橢圓 時(shí)間: 2025-3-23 10:06
Submm Continuum Observations of Sources from the I R A S Point-Source CatalogueIR data and extensive model fits over this large spectral range allow the determination of the total luminosity, dust temperatures, the wavelength dependence of dust opacity, the total amount of extinction towards embedded stellar objects and the density distribution of dust around central heating s作者: rectocele 時(shí)間: 2025-3-23 14:06
A Statistical Analysis of the LRS Catalogs types of spectra (LRS classes) can readily be associated with well-known groups of objects. About 96% of the sources are stars, most of them with oxygen- or carbon-rich envelopes, five sources are galaxies, and the others are compact HII regions, planetary nebulae, and ‘peculiar stars’.作者: 騷動(dòng) 時(shí)間: 2025-3-23 18:36
The Zodiacal Background in the IRAS Datamicrometers. These data provide insights into the character, spatial distribution, and perhaps origin of these particles which both confirm and expand upon those gained from previous zodiacal light studies. The zodiacal emission is a major component of the large scale infrared brightness of the sky 作者: RAFF 時(shí)間: 2025-3-23 23:03
Heliocentric Dependences of Zodiacal Emission, Temperature and Albedo are retrieved from IRAS data (Hauser et al., 1984) in two localized regions of the line-of-sight, near 0.98 and 1.40 a.u. heliocentric distance. The model-dependence is reduced, compared to the values averaged on the line-of-sight. The temperature probably does not exceed 250 K at the distance of t作者: 濃縮 時(shí)間: 2025-3-24 05:21 作者: 噴出 時(shí)間: 2025-3-24 07:44 作者: 鈍劍 時(shí)間: 2025-3-24 10:50
Dust at the North Galactic Polemag. The reddened areas may be organized in parallel string-like features. The IRAS clouds B and C are located in the NGP zone and a reasonable agreement is obtained for the 100μ intensities estimated from the optical absorption observations and the infrared emission measurements. It is further indi作者: Angioplasty 時(shí)間: 2025-3-24 16:58 作者: 努力趕上 時(shí)間: 2025-3-24 20:44 作者: 執(zhí)拗 時(shí)間: 2025-3-25 01:57
A Search for Infrared Excesses in G-Type Starsified, 15 have enhanced emission at λ > 25 μm. This group includes 4 supergiants, 8 variable stars, and 3 stars known to have dusty circumstellar medii (RU Cen, R Sge, HD-101584). The preliminary findings from this study are described.作者: Acetaminophen 時(shí)間: 2025-3-25 06:26
IRAS Intrinsic Colours of Hot Starsny of the O, B and A stars have excess fluxes at 12 μm. From a comparison of the relation to models we conclude that: a) The extrapolation of the Kurucz (1979) models from the visual to 12 μm results in a 12 μm flux that is about 10 percent too low, and b) The energy distribution for hot stars from 作者: Extemporize 時(shí)間: 2025-3-25 10:40 作者: intangibility 時(shí)間: 2025-3-25 12:14
Dust Formation in Wolf-Rayet Stellar Windsnded by dust shells. Apart from episodic and variable dust formation around some late WC stars, most WC8, WC8.5, WC9, and WC10 stars show a constant termal IR excess over the history of IR astronomy..In the past four years all 28 galactic WC stars of those types were monitored from ESO and UKIRT. Th作者: 2否定 時(shí)間: 2025-3-25 18:21
antly, for professors and students of psychology as well. It is critically necessary for psychologists to learn from their colleagues who are working in different cultural contexts in order to develop the type of knowledge and psychological understanding of human behavior that will be maximally usef作者: 沐浴 時(shí)間: 2025-3-25 20:30 作者: 衣服 時(shí)間: 2025-3-26 02:31 作者: Vital-Signs 時(shí)間: 2025-3-26 06:31 作者: 嘲弄 時(shí)間: 2025-3-26 10:43 作者: FAST 時(shí)間: 2025-3-26 15:26
T. N. Gautiern Personalverm?gen interpretieren lassen, die sie im vereinbarten arbeitsvertraglichen Umfang einem Unternehmen zur Nutzung zur Verfügung stellen. Diese stellen neben dem Sachverm?gen einen zentralen Faktor zur unternehmerischen Leistungserstellung und somit zur Realisierung des Unternehmenserfolges作者: Dawdle 時(shí)間: 2025-3-26 18:48
F. C. Gillettdlicher Perspektive dem Thema Corporate Governance widmet. Die Schwerpunkte in diesen Analysen sind sehr unt- schiedlich gesetzt. Zudem ist das Gebiet Corporate Governance dadurch gepr?gt, das eine Reihe unterschiedlicher Disziplinen (Betriebswirtschaftslehre, Volkswirtschaf- lehre, Soziologie, Rech作者: 揉雜 時(shí)間: 2025-3-27 00:22 作者: instulate 時(shí)間: 2025-3-27 03:11
S. F. Odenwald Einheit t?tig werden.. Sie stellen daher ein Beispiel für eine kommunale Serviceeinheit im Sinne dieser Untersuchung dar. Neben den Bereichen Hoch- und Tiefbau, Gartenunterhaltung sowie Bauunterhaltung sind Bauh?fe der technischen Bauverwaltung zuzuordnen.. In diesem Komplex besteht die Tendenz, fa作者: 持久 時(shí)間: 2025-3-27 05:26 作者: Rustproof 時(shí)間: 2025-3-27 11:54 作者: 神刊 時(shí)間: 2025-3-27 13:50
Dust Formation in Wolf-Rayet Stellar Windsof the large mass loss rates, of the order of 3.10. M./yr, the high density winds carry the dust away. Since in most cases the IR characteristics are constant over many years, this implies that the dust is constantly being replenished..In modeling the IR observations, (ρ,T) criteria are derived for 作者: RLS898 時(shí)間: 2025-3-27 18:22
Conference proceedings 1986ws of the conference center. Parallel to the IRAS Conference, a Workshop on Infrared Properties of Interstellar Grains was organized by J. M. Greenberg of the Leiden Laboratory Astrophysics Group: a busy shuttling of participants between the Workshop room and the Main Conference Hall showed that man作者: idiopathic 時(shí)間: 2025-3-27 22:24
ocial factors in different countries frame individual experience and affect the science and practice of psychology. Each of the chapters will provide a content-specific overview of how the curriculum in psychology with regards to social, development, clinical, counseling psychology, etc will need to作者: 個(gè)人長(zhǎng)篇演說 時(shí)間: 2025-3-28 05:27 作者: HERTZ 時(shí)間: 2025-3-28 06:58 作者: Inclement 時(shí)間: 2025-3-28 12:15 作者: 能量守恒 時(shí)間: 2025-3-28 16:59 作者: Binge-Drinking 時(shí)間: 2025-3-28 20:26
T. N. Gautieri diesem Verst?ndnis in einer m?glichst optimalen Beseitigung von Knappheitssituationen, bezogen auf die zur unternehmerischen Leistungserstellung ben?tigten Qualifikationen und Motivationen der Mitarbeiter unter Beachtung ?konomischen Denkens. Die Umsetzung ?konomischen Denkens führt zum ?konomisch作者: malign 時(shí)間: 2025-3-28 23:00
F. C. Gillett an einer Reihe von Gründen liegen, die sowohl methodischer als auch inhaltlicher Natur sind. Hier liegt die zentrale Fragestellung, der sich Frau Z?llner in der vorliegenden Arbeit widmet. Die Zusammenh?nge zwischen Corporate Governance und Unternehmenserfolg struk- riert darzustellen, um hieraus Handlungsem978-3-8350-0884-7978-3-8350-5444-8作者: Mindfulness 時(shí)間: 2025-3-29 05:55 作者: 愉快么 時(shí)間: 2025-3-29 08:14 作者: opalescence 時(shí)間: 2025-3-29 15:28
J. Coté,L. B. F. M. Watersr?gung des Bereichs schafft zudem günstige Voraussetzungen für betriebswirtschaftlich ausgerichtete Reformans?tze. Somit handelt es sich hierbei um den Teil der Kommunalverwaltung, in dem Reformelemente wie dezentrale Ressourcenverantwortung, Kontraktmanagement oder der Wettbewerb mit der Privatwirt作者: overreach 時(shí)間: 2025-3-29 17:22
0067-0057 . Greenberg of the Leiden Laboratory Astrophysics Group: a busy shuttling of participants between the Workshop room and the Main Conference Hall showed that man978-94-010-8577-9978-94-009-4672-9Series ISSN 0067-0057 Series E-ISSN 2214-7985 作者: BLA 時(shí)間: 2025-3-29 20:28 作者: 殺菌劑 時(shí)間: 2025-3-30 01:01 作者: 凈禮 時(shí)間: 2025-3-30 05:58 作者: Ischemia 時(shí)間: 2025-3-30 10:45 作者: 涂掉 時(shí)間: 2025-3-30 16:17
A Statistical Analysis of the LRS Catalogs types of spectra (LRS classes) can readily be associated with well-known groups of objects. About 96% of the sources are stars, most of them with oxygen- or carbon-rich envelopes, five sources are galaxies, and the others are compact HII regions, planetary nebulae, and ‘peculiar stars’.作者: Ingenuity 時(shí)間: 2025-3-30 19:29
Spectral Decomposition of IRAS Mapsm cold interstellar dust at ~ 20 K. The confusion due to this background tends to obscure other, weaker emission, such as e.g. the emission from the shock-heated dust (T ~ 60 K) we have been looking for in supernova remnants (Braun et al 1986).作者: Pamphlet 時(shí)間: 2025-3-31 00:15 作者: Carminative 時(shí)間: 2025-3-31 02:57 作者: SLUMP 時(shí)間: 2025-3-31 07:37
A Statistical Analysis and Overview of the IRAS Point Source CatalogThe IRAS Point Source Catalog can be segregated into stars, “IR galactic components”, galaxies, cirrus, and “disk and bulge stars” categories. For each source type, the types and distances of the sources are discussed, and the sky distribution, log N/log S, and identification rate are given.作者: 谷物 時(shí)間: 2025-3-31 09:13
The Infrared Excess From Stellar WindsThe IR excess can be used to study the density or velocity structure in the lower parts of the winds of early type stars. The depth of the emitting region and the excess in magnitudes is given for typical O-stars, as a function of λ and ?. The first results of an ongoing study of the IRAS data are discussed briefly.作者: 陳舊 時(shí)間: 2025-3-31 15:54
IRAS Observations of Wolf-Rayet StarsIRAS PSC, LRS, and CPC observations of Wolf-Rayet stars are used as diagnostics of hot circumstellar dust shells, cool dust in WR ring nebulae, the Ne/He abundance ratio, and the interstellar extinction. In two cases the IR energy distributions indicate WR planetary nucleus status rather than Population-I WR status.作者: Indebted 時(shí)間: 2025-3-31 17:51
Astrophysics and Space Science Libraryhttp://image.papertrans.cn/l/image/586081.jpg作者: Kidney-Failure 時(shí)間: 2025-3-31 23:42
978-94-010-8577-9D. Reidel Publishing Company, Dordrecht, Holland 1986
