標(biāo)題: Titlebook: Dark Matter in Astro- and Particle Physics; Proceedings of the I H. V. Klapdor-Kleingrothaus,R. D. Viollier Conference proceedings 2002 Spr [打印本頁] 作者: 評估 時間: 2025-3-21 18:19
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書目名稱Dark Matter in Astro- and Particle Physics被引頻次
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書目名稱Dark Matter in Astro- and Particle Physics讀者反饋
書目名稱Dark Matter in Astro- and Particle Physics讀者反饋學(xué)科排名
作者: Androgen 時間: 2025-3-21 20:17
The Dark Mass at the Center of the Milky Waybital accelerations for some of the most central stars of our Galaxy confirming the results obtained by Ghez et al. (2000) with NIRC at the Keck telescope. A detailed analysis combining the high precision but shorter time scale NIRC/Keck data with the lower precision but longer time scale SHARP/NTT 作者: 心痛 時間: 2025-3-22 03:38
Dim Matter in the Disks of Low Surface Brightness Galaxiestions due to the various components of the galaxies. For this purposegalaxies are selected which show clear spiral structure. Arguments of density wave theory of galactic spiral arms are then used to estimate the masses of the galactic disks. These estimates seem to indicate that the disks of low su作者: detach 時間: 2025-3-22 04:37
Black Holes in Active Galactic Nucleithe galaxian matter from its vicinity. The release of the gravitational energy of the infalling matter is ultimately responsible for the large radiative output of those objects, and in some cases, for formation and acceleration of powerful relativistic jets. This paper outlines our current understan作者: harmony 時間: 2025-3-22 12:11 作者: contrast-medium 時間: 2025-3-22 15:33 作者: contrast-medium 時間: 2025-3-22 17:29
Baryonic Dark Matter and Machosr halo consisting of baryons in the form of Machos is ruled out, leaving an elementary particle as the prime candidate for the dark matter. The observed microlensing events may make up around 20% of the dark matter in the Milky Way, or may indicate an otherwise undetected component of the Large Mage作者: 狂怒 時間: 2025-3-23 01:15 作者: 白楊 時間: 2025-3-23 03:04
icipants gave very nice professional talks during the conference. We are grateful to John Ellis for doing an incredible job preparing his excellent summary talk during the sessions. Some specia978-3-642-62920-4978-3-642-55739-2作者: overhaul 時間: 2025-3-23 08:13
The Dark Mass at the Center of the Milky Wayly inclined (60° < . < 80°), and eccentric (0.4 < . < 0.95) orbits around a central dark mass. The combination of both data sets results in a position of this central mass of .. E and .. S of the nominal radio position of Sgr A.. In particular it is possible to statistically correct the observed acc作者: 舊病復(fù)發(fā) 時間: 2025-3-23 10:38
Comparison of the Black Hole and Fermion Ball Scenarios of the Galactic Centernd eventually rule out one of the currently acceptable scenarios. This could shed some light on the nature of the supermassive compact dark object, or dark matter in general, at the center of our Galaxy.作者: encomiast 時間: 2025-3-23 17:28
Aufgaben aus der Theoretischen Physikly inclined (60° < . < 80°), and eccentric (0.4 < . < 0.95) orbits around a central dark mass. The combination of both data sets results in a position of this central mass of .. E and .. S of the nominal radio position of Sgr A.. In particular it is possible to statistically correct the observed acc作者: AER 時間: 2025-3-23 20:57
Aufgaben aus der Theoretischen Physiknd eventually rule out one of the currently acceptable scenarios. This could shed some light on the nature of the supermassive compact dark object, or dark matter in general, at the center of our Galaxy.作者: Counteract 時間: 2025-3-23 23:45 作者: 高談闊論 時間: 2025-3-24 02:49 作者: impale 時間: 2025-3-24 10:09 作者: temperate 時間: 2025-3-24 11:16
Aufgaben aus der Technischen Mechanikdensity parameter from redshift space distortions in galaxy surveys, and show evidence for similar streaming motions of clusters in the REFLEX redshift-space correlation function ξ(.., π). The overall picture shows a remarkable consistency of independent clustering data and measurements towards the same low-density CDM model with ..作者: 吹牛需要藝術(shù) 時間: 2025-3-24 16:06 作者: MOTTO 時間: 2025-3-24 21:40
Aufgaben aus der technischen Mechanikts toward the LMC over the next 5 years. The expected discovery of a number of microlensing events exhibiting special properties due to binarity, etc., will allow us to better determine the location and nature of the lenses causing the LMC microlensing events.作者: 確定方向 時間: 2025-3-25 01:26 作者: evaculate 時間: 2025-3-25 06:05 作者: 無價值 時間: 2025-3-25 09:01 作者: 同時發(fā)生 時間: 2025-3-25 11:39 作者: Congregate 時間: 2025-3-25 17:07
Aufgaben aus der Theoretischen Physikosmic structures. Extra-heating from Supernovae following star formation in the galaxies which built up the groups/clusters can account for the observations in a . dominated or in a critical Universe, while they fail to provide the observed X-ray properties of galaxy groups in open Universes or in models with a high fraction of hot dark matter ..作者: ascend 時間: 2025-3-25 23:44
Dark Matter and Baryons in Groups and Clusters of Galaxiesosmic structures. Extra-heating from Supernovae following star formation in the galaxies which built up the groups/clusters can account for the observations in a . dominated or in a critical Universe, while they fail to provide the observed X-ray properties of galaxy groups in open Universes or in models with a high fraction of hot dark matter ..作者: Increment 時間: 2025-3-26 00:21
held in Cape Town, South Africa, in the period 4-9 February 2002. This majestic natural area was the site of the first conference of this series (hosted since 1996 in Heidelberg) to be held outside of Germany. Dark Matter has become one of the most exciting and central fields of as- trophysics, par作者: 殘忍 時間: 2025-3-26 07:06
Aufgaben aus der Theoretischen Physikve output of those objects, and in some cases, for formation and acceleration of powerful relativistic jets. This paper outlines our current understanding of the structure of AGN, and summarizes the observational evidence for black holes in those objects.作者: Canyon 時間: 2025-3-26 12:12
Aufgaben aus der Theoretischen Physiked microlensing events may make up around 20% of the dark matter in the Milky Way, or may indicate an otherwise undetected component of the Large Magellanic Cloud. Several new pieces of work lend support to both possibilities, leaving the answer uncertain.作者: Yourself 時間: 2025-3-26 14:31
Aufgaben aus der Technischen Mechaniksults on the power spectrum and two-point correlation correlation function from the 2dF and REFLEX surveys, highlighting the advantage of X-ray clusters in the comparison to cosmological models, given their easy-to-understand mass selection function. I also mention recent measurements of the matter 作者: SKIFF 時間: 2025-3-26 18:19 作者: 有抱負(fù)者 時間: 2025-3-27 00:28 作者: 無目標(biāo) 時間: 2025-3-27 03:30 作者: JOT 時間: 2025-3-27 07:52 作者: legislate 時間: 2025-3-27 11:40
Aufgaben aus der Theoretischen Physikensity profiles of dark matter are approximatively self-similar (i.e., their shape do not depend on the mass scale), those of the gas (observable through its copious X-ray emission) become shallower for masses below ~ 5 x 10.....We show how such observed properties point toward pre-heating of the ga作者: 多余 時間: 2025-3-27 17:28
Aufgaben aus der Theoretischen Physikr halo consisting of baryons in the form of Machos is ruled out, leaving an elementary particle as the prime candidate for the dark matter. The observed microlensing events may make up around 20% of the dark matter in the Milky Way, or may indicate an otherwise undetected component of the Large Mage作者: Femish 時間: 2025-3-27 19:56 作者: Monolithic 時間: 2025-3-27 22:43 作者: PHON 時間: 2025-3-28 03:01 作者: 到婚嫁年齡 時間: 2025-3-28 10:02
H. V. Klapdor-Kleingrothaus,R. D. ViollierIncludes supplementary material: 作者: fiction 時間: 2025-3-28 11:20 作者: 起波瀾 時間: 2025-3-28 15:15
Koordination von Zuliefernetzwerkenped with inertial measurements units. Free-moving robotic systems could gain the full benefits of inertial measurements if the measurement units are placed on independently orientable platforms, such as a human-like heads. We illustrate these benefits by analysing recent humanoid robots design and control approaches.作者: Senescent 時間: 2025-3-28 18:46
U. Ackermann Hamiltonian Systems and Celestial Mechanics 2014" (HAMSYS2014) (15 abstracts) and at the "Workshop on Virus Dynamics and Evolution" (12 abstracts), both held at the Centre de Recerca Matemàtica (CRM) in Barcelona from June 2nd to 6th, 2014, and from June 23th to 27th, 2014, respectively. Most of th作者: Lucubrate 時間: 2025-3-29 02:05
