標(biāo)題: Titlebook: Galaxies and their Masks; A Conference in Hono David L. Block,Kenneth C. Freeman,Ivanio Puerari Conference proceedings 2010 Springer Scienc [打印本頁(yè)] 作者: Tyler 時(shí)間: 2025-3-21 17:19
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作者: Banquet 時(shí)間: 2025-3-21 22:02
Kenneth Lyons Jones,H. Eugene Hoymeuch as rings, nuclear arms, nuclear bars, and asymmetries. We find a centrally peaked concentration in about 85% of the galaxies with typical size scales of about 0.5–1 kpc. This might be related to perturbations produced by recent interactions.作者: 情節(jié)劇 時(shí)間: 2025-3-22 01:11 作者: 飛行員 時(shí)間: 2025-3-22 06:38 作者: 使虛弱 時(shí)間: 2025-3-22 10:12 作者: LEERY 時(shí)間: 2025-3-22 16:12
Sonal,Sharmita Gupta,Yati Prabha,S. K. Sonillicity gradient, bars with null metallicity gradient, and galaxies with positive metallicity gradient. Regarding the bulge region we find that the ages and metallicities are younger and more metal rich, at a given ., than the bulges of unbarred galaxies. The bulges of the barred galaxies in our sam作者: LEERY 時(shí)間: 2025-3-22 17:15 作者: obeisance 時(shí)間: 2025-3-23 01:04 作者: 組成 時(shí)間: 2025-3-23 04:43 作者: PHIL 時(shí)間: 2025-3-23 08:05
The Large Magellanic Cloud: A Power Spectral Analysis of Spitzer Images,similar to the in-plane velocities at small scales. The motions are highly anisotropic at large scales,with in-plane velocities being much more important than vertical ones.In contrast, at small scales, the motions become more isotropic.作者: Presbycusis 時(shí)間: 2025-3-23 12:33
What Can the Radial Surface Brightness Profiles of Galaxy Discs Tell Us About Their Evolution?,ere the inner disc slope changes to a more abrupt outer slope have increased with epoch, but that at all epochs this radius has the bluest, i.e. the youngest stellar population. This can be explained via models which combine stellar migration due to non-axisymmetry with continuous star formation due作者: 類(lèi)人猿 時(shí)間: 2025-3-23 15:50
Bars and Bulges Through Masks of Time,llicity gradient, bars with null metallicity gradient, and galaxies with positive metallicity gradient. Regarding the bulge region we find that the ages and metallicities are younger and more metal rich, at a given ., than the bulges of unbarred galaxies. The bulges of the barred galaxies in our sam作者: 聽(tīng)寫(xiě) 時(shí)間: 2025-3-23 19:14
Conference proceedings 2010e of planet’s most highly cited astronomers. The current volume affords readers a unique perspective on galaxies by probing the thoughts of some of the greatest astronomers of our age. Contributions focus on galaxies from within our Local Group to those in our high redshift Universe. Approximately 4作者: 暖昧關(guān)系 時(shí)間: 2025-3-24 00:17 作者: 有罪 時(shí)間: 2025-3-24 03:42
astronomers Contains over 200 color images.Includes supplemVarious kinds of masks obscure our view of our galaxy, the Milky Way, as well as of other galaxies. Masks of interstellar dust affect our measurements within galaxies, on scales ranging from individual supernovae to the galaxies themselves.作者: 漫步 時(shí)間: 2025-3-24 07:29 作者: jagged 時(shí)間: 2025-3-24 13:36 作者: Barter 時(shí)間: 2025-3-24 15:21
Advances in Pharmaceutical Biotechnologyk matter and lead to the conclusion that disks are in general not “maximal”, have lower . ratios than previously suspected, and are locally stable w.r.t. Toomre’s . criterion for local stability. I will end with a few words on “truncations” in stellar disks.作者: delegate 時(shí)間: 2025-3-24 19:28
Artificial Chlorophyll-Protein Complexesst results on modelling the dust content of edge-on spiral galaxies using both optical and Herschel far-infrared data. Both of these results demonstrate the complex interplay of dust and star light in spiral galaxies.作者: 無(wú)聊點(diǎn)好 時(shí)間: 2025-3-25 01:47 作者: Spongy-Bone 時(shí)間: 2025-3-25 06:17
Advances in Physiological Researches of their hostgalaxy. We briefly discuss how upcoming observations, e.g., imaging from the . Survey of Stellar Structure in Galaxies (S.G), will lead to significant further advances in this area of research.作者: 信徒 時(shí)間: 2025-3-25 07:55
Rings and Bars: Unmasking Secular Evolution of Galaxies,es of their hostgalaxy. We briefly discuss how upcoming observations, e.g., imaging from the . Survey of Stellar Structure in Galaxies (S.G), will lead to significant further advances in this area of research.作者: minion 時(shí)間: 2025-3-25 12:36 作者: 濃縮 時(shí)間: 2025-3-25 16:23
Light Cores Behind Dark Masks,hich the dynamically cold gaseous component is rapidly converted into a dynamically hot stellar component. Meanwhile only a small fraction of the gas contributes to the growth of the off-centered compact object.作者: frenzy 時(shí)間: 2025-3-25 20:37
Conference proceedings 2010 within galaxies, on scales ranging from individual supernovae to the galaxies themselves. The “mass mask” (our inability to image mass rather than light) gives astronomers a very incomplete picture of the size and structure of galaxies themselves, because we cannot image the dark matter which provi作者: Anonymous 時(shí)間: 2025-3-26 02:49 作者: 使出神 時(shí)間: 2025-3-26 07:14
Globalization, Open Access Publishing, and the Disappearance of Print: Threat or Opportunity?, between libraries. Old business models are being replaced by new business models, such as open access publishing. The familiar print format is disappearing for journals and perhaps for books. This chapter presents an overview of these developments and addresses potential threats and opportunities to the parties involved in publishing.作者: Radiculopathy 時(shí)間: 2025-3-26 12:23
Structure, Mass, and Stability of Galactic Disks,k matter and lead to the conclusion that disks are in general not “maximal”, have lower . ratios than previously suspected, and are locally stable w.r.t. Toomre’s . criterion for local stability. I will end with a few words on “truncations” in stellar disks.作者: Ophthalmoscope 時(shí)間: 2025-3-26 13:24 作者: hemophilia 時(shí)間: 2025-3-26 18:52 作者: 團(tuán)結(jié) 時(shí)間: 2025-3-26 22:07 作者: PATHY 時(shí)間: 2025-3-27 03:33 作者: Anonymous 時(shí)間: 2025-3-27 06:55 作者: 該得 時(shí)間: 2025-3-27 12:35 作者: 要塞 時(shí)間: 2025-3-27 14:45
Erdogan Madenci,Pranesh Roy,Deepak Beheragh this halo medium. Since the dwarfs are stripped at distances generally greater than 20 kpc, the gas is unlikely to make it directly into the spiral galaxy disk as cold star formation fuel. Some of the dwarfs’ gas may be integrated into the spiral galaxy’s hot halo and warm clumps may undergo a recooling process close to the disk.作者: 尖叫 時(shí)間: 2025-3-27 18:51
Lars Schweizer,Theodor Dingermannrived SN rates used for providing an independent measurement of the SF history of the Universe. We also present thus far the first NIR luminosity functions of super star cluster (SSC) candidates. The LFs can then be used to constrain the formation and evolution of SSCs via constraints based on initial mass functions and cluster disruption models.作者: arboretum 時(shí)間: 2025-3-28 01:23 作者: sperse 時(shí)間: 2025-3-28 05:03 作者: coagulation 時(shí)間: 2025-3-28 08:50 作者: 即席演說(shuō) 時(shí)間: 2025-3-28 12:52
The Mask of Complexity in Disk Galaxies, of galaxies; only with such a complexity reduction we can claim to understand what are galaxies. Thus complexity acts as a mask which can be sometimes removed, unveiling the hidden simplicity of galaxies.作者: 預(yù)防注射 時(shí)間: 2025-3-28 15:39 作者: 捐助 時(shí)間: 2025-3-28 20:40
Super Star Clusters and Supernovae in Interacting LIRGs Unmasked by NIR Adaptive Optics,rived SN rates used for providing an independent measurement of the SF history of the Universe. We also present thus far the first NIR luminosity functions of super star cluster (SSC) candidates. The LFs can then be used to constrain the formation and evolution of SSCs via constraints based on initial mass functions and cluster disruption models.作者: 抗體 時(shí)間: 2025-3-28 22:54 作者: inveigh 時(shí)間: 2025-3-29 06:00 作者: Brain-Imaging 時(shí)間: 2025-3-29 10:10
Twin Masks of Spiral Structure? A Local Perspective,metry of the Galaxy’s spiral arms, often with conflicting results. While a general consensus exists that a global pattern exists, considerable disagreement remains in the details. Arm geometries, orientations, and even the number of arms are still debated. Close examination of the literature reveals作者: Insul島 時(shí)間: 2025-3-29 14:04 作者: 完成才會(huì)征服 時(shí)間: 2025-3-29 16:12 作者: Range-Of-Motion 時(shí)間: 2025-3-29 23:26 作者: 忙碌 時(shí)間: 2025-3-30 03:38
Molecular Gas Properties of Galaxies: The SMA CO(2-1) B0DEGA Legacy Project,ogies in the circumnuclear regions. While in samples of “normal” galaxies the molecular gas does not seem to peak toward the nuclear regions for about 50% of the galaxies, barred galaxies and mergers show larger concentrations. However, we do not exactly know from an observational point of view how 作者: neuron 時(shí)間: 2025-3-30 04:14
,The DiVA’s Mask: Iconifying Galaxies and Revealing HI Anomalies,ibution and velocity behaviour of HI emission using the 3-D information in data cubes. We explore creating 3-D masks from model galaxy cubes generated using parameters determined by GalAPAGOS. We call our technique of applying these masks to the original HI data cubes, and subsequent analysis of the作者: 低三下四之人 時(shí)間: 2025-3-30 08:33
Enigmatic Masks of Cosmic Dust: Lessons from Nearby Galaxies Through the Eyes of the Spitzer Space ters photographed with the Crossley reflector.Publications of the Lick Observatory, XIII, 11–42), was the prevalence of characteristic dark bands or streaks across the disk of the galaxies. These dark bands were interpreted to be lanes of light obscuring “occulting material”. While being nothing mor作者: 關(guān)節(jié)炎 時(shí)間: 2025-3-30 13:17
The Large Magellanic Cloud: A Power Spectral Analysis of Spitzer Images,ws.At larger scales (kpc) the slope is ~ ?1.6, while at smaller ones (tens to few hundreds of parsecs) the slope is steeper, with avalue ~ ?2.9.The break occurs at a scale ~ 100 ? 200 pc. We interpret this break as the scale height of the dust disk of the LMC. We perform high-resolution simulations 作者: Functional 時(shí)間: 2025-3-30 17:07
Light Cores Behind Dark Masks,ck hole and the host galaxy bulge mass. Two of the nearest spiral galaxies with nuclear starburst host off-centered compact cores associated with the peak of the infrared emission.These compact objects are lightweight, up to a few million solar masses. Their locations imply that they are triggering 作者: 挖掘 時(shí)間: 2025-3-31 00:46
Globalization, Open Access Publishing, and the Disappearance of Print: Threat or Opportunity?,ternet. The Internet has accelerated globalization, which in turn has enhanced the consolidation of commercial publishing houses and the collaboration between libraries. Old business models are being replaced by new business models, such as open access publishing. The familiar print format is disapp作者: 桉樹(shù) 時(shí)間: 2025-3-31 02:59
Super Star Clusters and Supernovae in Interacting LIRGs Unmasked by NIR Adaptive Optics,le interpretation of kinematic, dynamical and star formation (SF) properties of these very dusty objects.Whole progenitor nuclei in the interactions can be missed if only optical HST imaging is used. Here we specifically present the latest results regarding core-collapse supernovae found within the 作者: 陰險(xiǎn) 時(shí)間: 2025-3-31 05:14
Structure, Mass, and Stability of Galactic Disks,nd dynamics of stellar disks. Next I will review the progress in the area of flaring of H. layers. These subjects are relevant for the presence of dark matter and lead to the conclusion that disks are in general not “maximal”, have lower . ratios than previously suspected, and are locally stable w.r作者: 監(jiān)禁 時(shí)間: 2025-3-31 12:48 作者: 享樂(lè)主義者 時(shí)間: 2025-3-31 13:36 作者: etiquette 時(shí)間: 2025-3-31 19:56
Galaxy Morphology Revealed By SDSS: Blue Elliptical Galaxies, some insights into the formation and evolution of galaxies. There seems to be two types of blue elliptical galaxies. One type shows globally blue colors suggesting star formations over the entire galaxy whereas the other type shows blue core that indicates enhanced star formation in the nuclear reg
