標(biāo)題: Titlebook: Mapping the Galaxy and Nearby Galaxies; Keiichi Wada,Fran?oise Combes Conference proceedings 2008 Springer-Verlag New York 2008 Galaxy For [打印本頁(yè)] 作者: 烤問(wèn) 時(shí)間: 2025-3-21 18:02
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書(shū)目名稱Mapping the Galaxy and Nearby Galaxies影響因子(影響力)學(xué)科排名
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書(shū)目名稱Mapping the Galaxy and Nearby Galaxies讀者反饋
書(shū)目名稱Mapping the Galaxy and Nearby Galaxies讀者反饋學(xué)科排名
作者: antiandrogen 時(shí)間: 2025-3-21 20:14
978-1-4419-2495-7Springer-Verlag New York 2008作者: harbinger 時(shí)間: 2025-3-22 04:07 作者: Aspiration 時(shí)間: 2025-3-22 08:04
Keiichi Wada,Fran?oise CombesThis is a proceedings book based on review and contributed talks presented in a recent conference.Readers (professional astronomers, graduate students, and scientific journalists) can learn recent obs作者: Left-Atrium 時(shí)間: 2025-3-22 10:22 作者: Decibel 時(shí)間: 2025-3-22 14:14
Dynamics of Stars in the Inner Galactic Bulge Revealed from SiO Maser Surveys s.. Based on numerical simulations of stellar orbits in the Galactic bulge, we conclude that the latter feature is created as a result of a past star formation in the bulge, when the intersecting point of the .. and .. orbits was considerably outside of the present position.作者: 本能 時(shí)間: 2025-3-22 20:04 作者: Adherent 時(shí)間: 2025-3-22 22:58
Mapping Circumnuclear Dust in Nearby Galaxiesre feedback processes in galaxies appear to have substantially affected the morphology and kinematics of the circumnuclear ISM and discuss the implications of this work for future studies, particularly with ALMA.作者: endoscopy 時(shí)間: 2025-3-23 03:08
1570-6591 e students, and scientific journalists) can learn recent obsIn our quest to elucidate the origin of the universe and the formation of galaxies, particularly that of the Milky Way in which we live, astounding progress has been made in recent years through observational and theoretical studies. Not on作者: archaeology 時(shí)間: 2025-3-23 07:43 作者: Banquet 時(shí)間: 2025-3-23 09:48
Global MHD Simulations of Galactic Gas Disksscape of azimuthal magnetic flux amplified in the disk. The quasi-periodic reversals of azimuthal magnetic fields create a magnetically striped halo, in which azimuthal magnetic fields reverse their direction with height.作者: irreparable 時(shí)間: 2025-3-23 17:42 作者: 未成熟 時(shí)間: 2025-3-23 20:10
Conference proceedings 2008ogress has been made in recent years through observational and theoretical studies. Not only have gigantic surveys covering a large fraction of the sky brought statistics enlightening evolutionary paths of galaxies, but powerful instruments, such as radio interferometers and ground- and space-based 作者: aptitude 時(shí)間: 2025-3-24 01:52 作者: 可行 時(shí)間: 2025-3-24 04:36
Numerical Modeling of the ISM in the Galactic Center and DisksWe find that the observed SFR in normal and starburst galaxies are well-fitted by the theoretical SFR in a wide range of the global gas density (10 –10..⊙pc.). Star formation efficiency (SFE) for high density gas (.>10. cm.) may be intrinsically different between starburst and normal galaxies.作者: 影響深遠(yuǎn) 時(shí)間: 2025-3-24 06:39
The Parkes Galactic Meridian Survey (PGMS) polarized synchrotron emission can be also investigated. This will be crucial for CMB Polarization observations, for which such Galactic emission acts as foreground noise. Here we present the survey together with some preliminary results.作者: Cardiac 時(shí)間: 2025-3-24 11:59
Mapping the Milky Way and the Local Grouproper motions of Local Group galaxies are now being measured. These observations will lead to direct mapping of the structure of the Milky Way, testing of the spiral density wave paradigm, measuring the dark matter halos of Local Group galaxies, and better understanding of the past history and future fate of these galaxies.作者: fructose 時(shí)間: 2025-3-24 18:22
Mapping Large-scale Magnetic Fields in Giant Molecular Cloudsh submillimeter polarimeters that have been operated from larger telescopes on Mauna Kea, SPARO obtains relatively coarse angular resolution but much better sensitivity to fainter, more extended emission. We have also discussed these recent SPARO observations in a paper in the Astrophysical Journal [3].作者: 藝術(shù) 時(shí)間: 2025-3-24 21:27 作者: 云狀 時(shí)間: 2025-3-25 01:35 作者: hegemony 時(shí)間: 2025-3-25 06:23
Mapping the Milky Way and the Local Grouprces separated by about 1° are being measured with accuracies of ~ 10 μas. With this accuracy, trigonometric parallaxes throughout the Milky Way and proper motions of Local Group galaxies are now being measured. These observations will lead to direct mapping of the structure of the Milky Way, testin作者: 恭維 時(shí)間: 2025-3-25 10:28 作者: miracle 時(shí)間: 2025-3-25 15:03
Dynamics of Stars in the Inner Galactic Bulge Revealed from SiO Maser Surveysities of ~160 detected objects. The longitude–velocity diagram of these objects reveals two conspicuous features: one indicating a linear velocity increase with longitude with |.| < 1.5°, which is likely to be associated with the inner bar, and the other having eccentric velocities with |..| >250 km作者: DEMN 時(shí)間: 2025-3-25 18:03
The Physics of Cold Gas in Galaxy Low Excitation Regionsiate to return considering the simplest situations. The low excitation regions in or around galaxies, such as the galaxy outer disks, the inter-arm regions, the well shielded starless cores in molecular clouds, or the high velocity clouds (HVC’), appear as ideally suited to test our understanding of作者: Trabeculoplasty 時(shí)間: 2025-3-25 23:32
Secular Evolution of Disc Galaxies and of their Componentsnsistent .-body simulations. When the bar forms, it is as thin as the disc. Its three-dimensional shape, however, evolves, so that, at later times, it has a thick inner part and a thin, more extended outer part. The former, when viewed edge-on, is called a boxy/peanut bulge, because of its shape. Th作者: Mammal 時(shí)間: 2025-3-26 01:27 作者: 紅潤(rùn) 時(shí)間: 2025-3-26 05:38 作者: 并排上下 時(shí)間: 2025-3-26 11:25 作者: 喚醒 時(shí)間: 2025-3-26 14:25
Numerical Modeling of the ISM in the Galactic Center and Disksscussed. 3-D hydrodynamic simulations show that the PDFs in globally stable, inhomogeneous ISM in galactic disks are well fitted by a single log-normal function over a wide density range. The dispersion of the log-normal PDF (LN-PDF) is larger for more gas-rich systems, whereas the characteristic de作者: 陰謀小團(tuán)體 時(shí)間: 2025-3-26 19:56 作者: Anhydrous 時(shí)間: 2025-3-26 21:10 作者: 切碎 時(shí)間: 2025-3-27 04:17 作者: 成份 時(shí)間: 2025-3-27 06:07
The Shapes and Supersonic Motions of Molecular Cloudsluence on the shape of molecular clouds [5]. We analyzed a sample of more than 500 molecular clouds identified with the BU-FCRAO Galactic Ring Survey (YRS) data, and found that they are preferentially elongated along the Galactic plane. Their spin axes are randomly oriented; therefore, we conclude t作者: 有罪 時(shí)間: 2025-3-27 11:36
Millimeter Dust Continuum Emission as a Tracer of Molecular Gas in Galaxiesy in cold interstellar regions. CO observations have been so far the best way to trace molecular gas in external galaxies, but in low metallicity environments the gas mass deduced could be largely underestimated due to enhanced photodissociation of CO. In this context, using millimeter dust emission作者: 自由職業(yè)者 時(shí)間: 2025-3-27 14:40
Mapping Circumnuclear Dust in Nearby Galaxieson maps of their cold ISM. These circumnuclear dust structures are of substantial interest for the study of mass transport in galaxies, particular secular evolution, fueling central starbursts, and nuclear accretion onto supermassive black holes. In this review I concentrate on several instances whe作者: 宣傳 時(shí)間: 2025-3-27 18:10 作者: Crohns-disease 時(shí)間: 2025-3-28 01:20
Caroline Bot,F. Boulanger,M. Rubio,F. Rantakyroen Massenverteilungen des Abschn. 1.29 das einfachste Beispiel eines ausgedehnten K?rpers. Zum zweiten stellt die Dynamik des starren K?rpers einen besonders sch?nen Modellfall dar, an dem man die allgemeinen Prinzipien der kanonischen Mechanik ausprobieren und die Folgerungen aus den jeweiligen r?u作者: 條街道往前推 時(shí)間: 2025-3-28 02:32
Paul Martininterworfen sein m?gen, deren Bewegung aber nicht durch zus?tzliche Bedingungen (wie die Vorgabe von starren Abst?nden, von Kurven, entlang derer einzelne Massenpunkte gleiten sollen, Begrenzungsfl?chen und dergleichen) eingeschr?nkt sind. Das bedeutet, da? man solche mechanischen Systeme direkt mit 作者: 看法等 時(shí)間: 2025-3-28 07:35 作者: BIAS 時(shí)間: 2025-3-28 10:44 作者: PANEL 時(shí)間: 2025-3-28 15:00
The Physics of Cold Gas in Galaxy Low Excitation Regionsuring this cold phase are important since they determine the fate of almost everything we can observe..But precisely because the lack of excitation prevents various radiative emissions to occur, cold gas is difficult to observe. Most matter is then neutral and at the lowest energy levels. The restri作者: follicle 時(shí)間: 2025-3-28 22:21 作者: 槍支 時(shí)間: 2025-3-29 01:42
Galactic Magnetic Fieldshe large-scale magnetic fields in the Galaxy and their direction. ‘Cosmic magnetismn‘ is one of the key-science projects for the planned Sqare Kilometre Array (SKA), which is based on a sensitive RM sky survey with an unprecedented high source density. The analysis of these data will provide magneti作者: 不來(lái) 時(shí)間: 2025-3-29 03:42 作者: MARS 時(shí)間: 2025-3-29 08:50
Conference proceedings 2008es? What causes starburst and AGN activity in galaxies? In order to discuss and make progress on these important questions, aided by recent observational and theoretical work, we organized a symposium en- tled “Mapping the Galaxy and Nearby Galaxies”, on 26 June - 30 June, 2006, at Ishigaki island. 作者: 裂隙 時(shí)間: 2025-3-29 14:58
Jin Koda daher darauf, den wichtigen Feldbegriff und die Verallgemeinerung der Prinzipien der kanonischen Mechanik für kontinuierliche Systeme einzuführen und durch Beispiele zu illustrieren. Gleichzeitig wird damit eine erste Grundlage für die Elektrodynamik bereitgestellt, die eine typische und besonders 作者: JAMB 時(shí)間: 2025-3-29 17:29 作者: prodrome 時(shí)間: 2025-3-29 21:53
Paul Martiniwischen Invarianzeigenschaften und Transformationen von Koordinatensystemen und Erhaltungss?tzen der Theorie auftreten, die sich als tragende Elemente der ganzen Mechanik herausstellen werden, ja, die wie ein cantus firmus . die ganze theoretische Physik durchziehen. Auch wird man schon in den erste作者: 圖畫(huà)文字 時(shí)間: 2025-3-30 01:56 作者: Immunoglobulin 時(shí)間: 2025-3-30 05:12
Mark Reid,Andreas Brunthaler,Xu Ye,Zheng Xing-Wu,Karl Menten,Lincoln Greenhill,Luca Moscadelli作者: 金桌活畫(huà)面 時(shí)間: 2025-3-30 11:16 作者: 保守黨 時(shí)間: 2025-3-30 15:13 作者: notice 時(shí)間: 2025-3-30 20:34
Ryoji Matsumoto,Hiromitsu Nishikori,Minoru Tanaka,Mami Machida作者: 協(xié)定 時(shí)間: 2025-3-31 00:13 作者: legacy 時(shí)間: 2025-3-31 02:47
