標題: Titlebook: Examining the Big Bang and Diffuse Background Radiations; Menas Kafatos,Yoji Kondo Book 1996 International Astronomical Union 1996 Gravity [打印本頁] 作者: Philanthropist 時間: 2025-3-21 19:02
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作者: 現(xiàn)存 時間: 2025-3-21 23:48
Measurement and Implications of the Cosmic Microwave Background Spectrumhe early universe. It also measured emission from nearby sources such as the stars, dust, molecules, atoms, ions, and electrons in the Milky Way, and dust and comets in the Solar System. It was launched 18 November 1989 on a Delta rocket., carrying one microwave instrument and two cryogenically cool作者: 碎石 時間: 2025-3-22 03:45 作者: 解脫 時間: 2025-3-22 06:17
Fluctuations In The Microwave Skyw have secure detections on some angular scales and improved upper limits on others. As the sensitivity of such searches increases, understanding sources of foreground noise (e.g., Galactic and extragalactic radio emission) becomes more important. Also reviewed are the contributions aperture synthes作者: 死貓他燒焦 時間: 2025-3-22 09:48 作者: Dendritic-Cells 時間: 2025-3-22 13:51 作者: Dendritic-Cells 時間: 2025-3-22 17:46 作者: Nonthreatening 時間: 2025-3-22 23:54
The Cobe Dirbe Search for the Cosmic Infrared Backgroundotropic cosmic infrared background radiation over the spectral range from 1.25 to 240 μm. The cumulative emissions of pregalactic, protogalactic, and evolving galactic systems are expected to be recorded in this background. The DIRBE instrument has mapped the full sky with high redundancy at solar e作者: 錯誤 時間: 2025-3-23 04:09
Degree Scale Anisotropy: Current Statusation of structure we now observe. Recent advances in degree scale anisotropy measurements have allowed us to begin critically testing cosmological models. Combined with the larger scale measurements from COBE we are now able to directly compare data and theory. These measurements promise future pro作者: 危機 時間: 2025-3-23 08:56
Galaxy Motions in The Nearby Universeof the field is that (1) convincing infall has been detected into dense clusters, especially the Virgo cluster, (2) the microwave background direction is moderately well aligned with the measured flow nearby but not apparently on larger scales, and (3) there is good but not perfect consistency betwe作者: 含水層 時間: 2025-3-23 12:52 作者: unstable-angina 時間: 2025-3-23 17:34 作者: 夾死提手勢 時間: 2025-3-23 20:15
International Astronomical Union Symposiahttp://image.papertrans.cn/e/image/318219.jpg作者: 橡子 時間: 2025-3-24 00:20 作者: Agnosia 時間: 2025-3-24 04:03
https://doi.org/10.57088/978-3-7329-9164-8Those of us who were around a few decades ago, frequently became initiated into cosmology by a very clear and concise small book, written by Herman Bondi, entitled “Cosmology” (1952/1960).作者: 極深 時間: 2025-3-24 09:50
Metafiguring Bollywood: Brecht after We review the main results obtained in the first cosmic experiment for study of the large scale anisotropy of CBR at 8 mm RELICT-1 and compare them with data of COBE mission.作者: Anthology 時間: 2025-3-24 13:56
Jeannette Littlemore,Graham LowDust, HI and molecular gas must be important components of distant radio galaxies. Recent observations to detect these constituents are discussed.作者: jaunty 時間: 2025-3-24 18:40
https://doi.org/10.1007/978-3-658-27650-8Detailed observations in the optical do not allow to discriminate between the following scenarii of galaxy formation:作者: 擴音器 時間: 2025-3-24 19:22
Mary Sanders Pollock,Catherine RainwaterDiffuse background radiation is integrated light which is consisted of various components of interplanetary, stellar, interstellar, galactic and intergalactic origins as well as cosmic background radiation, the remnant of the pre-galactic phenomena in the early history of the universe.作者: PSA-velocity 時間: 2025-3-25 00:10
https://doi.org/10.1057/9780230502215New observations obtained during the last two years have slightly shifted the balance of evidence towards larger values of H.. A compilation of recent determinations shows reasonable agreement and suggests that H. ? 75 km s. Mpc..作者: mechanical 時間: 2025-3-25 04:32
Introductory RemarksThose of us who were around a few decades ago, frequently became initiated into cosmology by a very clear and concise small book, written by Herman Bondi, entitled “Cosmology” (1952/1960).作者: 騷擾 時間: 2025-3-25 11:20 作者: 健談 時間: 2025-3-25 13:37 作者: 音樂會 時間: 2025-3-25 19:50 作者: 反抗者 時間: 2025-3-25 20:10 作者: PACT 時間: 2025-3-26 01:13
The Hubble Parameter — A Status Report at Epoch 1994.5New observations obtained during the last two years have slightly shifted the balance of evidence towards larger values of H.. A compilation of recent determinations shows reasonable agreement and suggests that H. ? 75 km s. Mpc..作者: sebaceous-gland 時間: 2025-3-26 08:18
978-0-7923-3815-4International Astronomical Union 1996作者: 輕浮思想 時間: 2025-3-26 10:19
Examining the Big Bang and Diffuse Background Radiations978-94-009-0145-2Series ISSN 1743-9213 Series E-ISSN 2352-2186 作者: Pde5-Inhibitors 時間: 2025-3-26 15:12
https://doi.org/10.1007/978-3-322-97217-0 year clearly peeled away all the sources to see a true background, if one even exists. All known backgrounds are astrophysically important and at least several cosmologically so. The path by which the standard hot big bang came to be generally regarded as standard is littered with the detritus of m作者: outer-ear 時間: 2025-3-26 20:30
Figurationen sp?tmoderner Lebensführunghe early universe. It also measured emission from nearby sources such as the stars, dust, molecules, atoms, ions, and electrons in the Milky Way, and dust and comets in the Solar System. It was launched 18 November 1989 on a Delta rocket., carrying one microwave instrument and two cryogenically cool作者: lavish 時間: 2025-3-27 00:23 作者: PHON 時間: 2025-3-27 02:03
Figurations of Human Subjectivityw have secure detections on some angular scales and improved upper limits on others. As the sensitivity of such searches increases, understanding sources of foreground noise (e.g., Galactic and extragalactic radio emission) becomes more important. Also reviewed are the contributions aperture synthes作者: 茁壯成長 時間: 2025-3-27 06:57 作者: 牛的細微差別 時間: 2025-3-27 09:38
Hans-Georg Soeffner,Dirk T?nzleria new 3-dimensional simulations of off-axis jet-cloud collisions. The results indicate that the most powerful radio sources are likely to be observed during or shortly after a jet-cloud interaction, and that such interactions can explain both the radio structures and the spatial association between作者: ABYSS 時間: 2025-3-27 15:55 作者: 激怒某人 時間: 2025-3-27 18:36
An Interview with Christine Lahtiotropic cosmic infrared background radiation over the spectral range from 1.25 to 240 μm. The cumulative emissions of pregalactic, protogalactic, and evolving galactic systems are expected to be recorded in this background. The DIRBE instrument has mapped the full sky with high redundancy at solar e作者: 我要威脅 時間: 2025-3-28 00:00
Eubulides, The Heap and The Euroation of structure we now observe. Recent advances in degree scale anisotropy measurements have allowed us to begin critically testing cosmological models. Combined with the larger scale measurements from COBE we are now able to directly compare data and theory. These measurements promise future pro作者: COUCH 時間: 2025-3-28 03:10 作者: 入伍儀式 時間: 2025-3-28 10:12
Zusammenfassung und Diskussion,the cosmic velocity of the cluster core is 1179 ± 17 km s., which, when combined with the distance gives H. = 55 ± 3 km s.Mpc. from the Virgo cluster data alone. Nine independent methods are reviewed that confirm that H. = 50 ± 2. Discussion is made why all methods that are said to give the short di作者: 使熄滅 時間: 2025-3-28 13:26 作者: 個阿姨勾引你 時間: 2025-3-28 17:15
Laboratorium Theater: Das Melodram,ates, with separations in the range 2–20 mas. None have been confirmed as lenses but several of them cannot yet. be definitively ruled out. If there are no milli-lenses in this sample then uniformly- distributed black holes of 10. to 10. M. cannot contribute more than ～ 1% of the closure density.作者: 后退 時間: 2025-3-28 20:30 作者: Permanent 時間: 2025-3-29 02:06 作者: ALOFT 時間: 2025-3-29 04:52
The Local Velocity Field And The Hubble Constantthe cosmic velocity of the cluster core is 1179 ± 17 km s., which, when combined with the distance gives H. = 55 ± 3 km s.Mpc. from the Virgo cluster data alone. Nine independent methods are reviewed that confirm that H. = 50 ± 2. Discussion is made why all methods that are said to give the short distance scale (H. ～ 85) are incorrect.作者: 微枝末節(jié) 時間: 2025-3-29 07:47
1743-9213 l Assembly in the Hague, Netherlands..The meeting attracted a large number - over 250 - ofastronomers, reflecting the strong interest engendered by the greatadvances in cosmology made in recent years. There is still a multitudeof unresolved problems in modern cosmology and the symposium offered awon作者: MIR 時間: 2025-3-29 12:12
https://doi.org/10.1007/978-3-322-97217-0st several cosmologically so. The path by which the standard hot big bang came to be generally regarded as standard is littered with the detritus of mistaken impressions, misunderstandings, and missed opportunities.作者: Coronation 時間: 2025-3-29 16:30 作者: 卵石 時間: 2025-3-29 19:47 作者: Ejaculate 時間: 2025-3-30 02:28 作者: Small-Intestine 時間: 2025-3-30 05:30
Of Cosmic Background Anisotropiesluding the geometry, topology, and dynamics of the Universe. Foreground galactic emissions, dust thermal emission and emission from energetic electrons, provide a serious limit to observations. Nevertheless, observations may determine if the evolution of the Universe can be understood from fundamental physical principles.作者: Defense 時間: 2025-3-30 09:05 作者: 烤架 時間: 2025-3-30 14:59
Figurations of Human Subjectivityis (interferometric) observations can make in characterizing cosmic background fluctuations and foreground sources of noise. Some recent results from the Very Large Array at . = 3.6 cm are given; these set a limit .T/T< 1.4 x 10-5 on fluctuations at . - 80. Recent work on the Sunyaev-Zel’dovich effect is summarized.作者: subacute 時間: 2025-3-30 17:55 作者: Militia 時間: 2025-3-30 20:56 作者: STALE 時間: 2025-3-31 03:50 作者: 大范圍流行 時間: 2025-3-31 06:33 作者: ADORN 時間: 2025-3-31 10:48 作者: 碳水化合物 時間: 2025-3-31 13:36
Book 1996 in the Hague, Netherlands..The meeting attracted a large number - over 250 - ofastronomers, reflecting the strong interest engendered by the greatadvances in cosmology made in recent years. There is still a multitudeof unresolved problems in modern cosmology and the symposium offered awonderful occ作者: Expediency 時間: 2025-3-31 19:05 作者: 四溢 時間: 2025-3-31 22:50 作者: Countermand 時間: 2025-4-1 03:59
Degree Scale Anisotropy: Current Statuseriments over the last six years using the ACME (Advanced Cosmic Microwave Explorer) payload which has made measurements at angular scales from 0.3 to 3 degrees and over a wavelength range from 1 to 10 mm. The recent data from these and other measurements will be reviewed as well as some of the chal作者: POINT 時間: 2025-4-1 08:08
Large-Scale Flows in The Local Universehese results bring into question the generally accepted reason for the peculiar velocities of galaxies that they arise solely as a consequence of infall into the dense regions of the universe. To the N. of the Great Attractor region, the flow increases and shows no sign of diminishing out to the red作者: Palpate 時間: 2025-4-1 10:43
Examining the Big Bang and Diffuse Background Radiations作者: Inscrutable 時間: 2025-4-1 17:09
