標題: Titlebook: Galaxy Interactions at Low and High Redshift; Proceedings of the 1 J. E. Barnes,D. B. Sanders Conference proceedings 1999 Springer Science+ [打印本頁] 作者: 分類 時間: 2025-3-21 17:37
書目名稱Galaxy Interactions at Low and High Redshift影響因子(影響力)
書目名稱Galaxy Interactions at Low and High Redshift影響因子(影響力)學(xué)科排名
書目名稱Galaxy Interactions at Low and High Redshift網(wǎng)絡(luò)公開度
書目名稱Galaxy Interactions at Low and High Redshift網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Galaxy Interactions at Low and High Redshift被引頻次
書目名稱Galaxy Interactions at Low and High Redshift被引頻次學(xué)科排名
書目名稱Galaxy Interactions at Low and High Redshift年度引用
書目名稱Galaxy Interactions at Low and High Redshift年度引用學(xué)科排名
書目名稱Galaxy Interactions at Low and High Redshift讀者反饋
書目名稱Galaxy Interactions at Low and High Redshift讀者反饋學(xué)科排名
作者: 不遵守 時間: 2025-3-21 22:51 作者: 無關(guān)緊要 時間: 2025-3-22 02:04
What can we Learn From the Local Group About the Role of Interactions in Galaxy Formation,the role of interactions in galaxy formation. Bulges are potentially of particular interest for galaxy formation because they are widely suspected to be the seeds for galaxy formation. Sites of active star formation at high redshift are often regarded as spheroids in the process of formation. In thi作者: 修飾 時間: 2025-3-22 08:04
The Magellanic Stream and The Magellanic Cloud System,eproduced the Magellanic Stream (Murai and Fujimoto 1980; Lin and Lynden-Bell 1982; Gardiner et al. 1994; Gardiner and Noguchi 1995; Lin et al. 1995), a narrow band of diffuse atomic hydrogen gas emerging from the SMC region, passing by the South Galactic Pole along an overhead great circle spanning作者: 口味 時間: 2025-3-22 08:46
The Nature and Fate of the Sagittarius Dwarf Galaxy,d into the Milky Way. This unique event allows the physics of galactic merging to be probed in unprecedented detail, and may shed light on the hypothesized population of primordial galaxies that merged to form the Milky Way.作者: burnish 時間: 2025-3-22 16:09 作者: burnish 時間: 2025-3-22 20:40 作者: 呼吸 時間: 2025-3-22 23:51
The Magellanic Stream Revisited,s in accordance with the Keplerian law at the distance of 50 kpc, while others have come to consider that the rotation curve of the Milky Way, essentially stays flat or is still increasing at the distance of the Magellanic Clouds and the Magellanic Stream.作者: Prosaic 時間: 2025-3-23 04:40
Are the Bulge C-Stars Related to the Sagittarius Dwarf Galaxy?,, are ideal tracers for such an event. Ng & Schultheis (1997) suggested that the Bulge carbon stars (Azzopardi et al. 1991; ALRW) might be at SDG’s distance. In the galactic Bulge these stars are completely different from carbon stars found in the LMC, SMC and dwarf spheroidal galaxies. If one keeps作者: PLUMP 時間: 2025-3-23 07:10 作者: Ordeal 時間: 2025-3-23 11:09 作者: Needlework 時間: 2025-3-23 17:18 作者: 注入 時間: 2025-3-23 19:45
A Near Infrared Survey of the LMC, bands. The observations were performed from Oct to Nov, 1994 at the Siding Spring Observatory. We used a 25 cm/F3.5 Newtonian telescope equipped with a 512x512 PtSi-Camera (Ueno et al. 1992). The plate scale was 4.″6 x 6.″0/pixel and the total field of view was 40.′2 x 52.′3. The system was attache作者: 天真 時間: 2025-3-24 01:58 作者: Soliloquy 時間: 2025-3-24 04:07 作者: 楓樹 時間: 2025-3-24 07:39 作者: Cervical-Spine 時間: 2025-3-24 13:11 作者: SNEER 時間: 2025-3-24 16:41
Extended Gas in Interacting Systems,s during an encounter, and the percentage of HI in the tails increases with the merging stage. However, the opposite is true for the molecular gas, which is observed highly concentrated towards the nuclei of interacting galaxies, amounting to a significant fraction of the dynamical mass. Statistical作者: 財政 時間: 2025-3-24 19:45
https://doi.org/10.1007/978-1-4612-0387-2 Observations of interacting galaxies at low redshifts (. ? 0.2) yield detailed information about many of the processes at work. I briefly review these processes and the growing evidence that mergers play a major role in the delayed formation of elliptical and early-type disk galaxies both in the fi作者: Pulmonary-Veins 時間: 2025-3-25 01:20 作者: mortgage 時間: 2025-3-25 03:26 作者: CESS 時間: 2025-3-25 09:08
The Female Epic: Antonine Maillet, ,eproduced the Magellanic Stream (Murai and Fujimoto 1980; Lin and Lynden-Bell 1982; Gardiner et al. 1994; Gardiner and Noguchi 1995; Lin et al. 1995), a narrow band of diffuse atomic hydrogen gas emerging from the SMC region, passing by the South Galactic Pole along an overhead great circle spanning作者: FOLLY 時間: 2025-3-25 13:04 作者: orthodox 時間: 2025-3-25 18:15 作者: 字謎游戲 時間: 2025-3-25 22:56 作者: 樹木中 時間: 2025-3-26 01:04
Esen ?zkaya,Kurtulu? Didem Yazgano?lus in accordance with the Keplerian law at the distance of 50 kpc, while others have come to consider that the rotation curve of the Milky Way, essentially stays flat or is still increasing at the distance of the Magellanic Clouds and the Magellanic Stream.作者: 背心 時間: 2025-3-26 08:21
Common Food Additives and Spices in Thailand, are ideal tracers for such an event. Ng & Schultheis (1997) suggested that the Bulge carbon stars (Azzopardi et al. 1991; ALRW) might be at SDG’s distance. In the galactic Bulge these stars are completely different from carbon stars found in the LMC, SMC and dwarf spheroidal galaxies. If one keeps作者: 索賠 時間: 2025-3-26 10:25 作者: Connotation 時間: 2025-3-26 13:41 作者: 惡名聲 時間: 2025-3-26 20:02
https://doi.org/10.1007/978-1-4302-3829-4stance information. Hypotheses range from supernova shells at 100 pc to intergalactic clouds at 1 Mpc. On statistical grounds, Blitz et al. (1996, ., ., 1349) claim that the HVCs are “remnants of Local Group formation, best explained as members of the Local Group of galaxies”. Reliable distances mus作者: 事與愿違 時間: 2025-3-26 21:56
An Optimum Supply-Demand Equilibrium?, bands. The observations were performed from Oct to Nov, 1994 at the Siding Spring Observatory. We used a 25 cm/F3.5 Newtonian telescope equipped with a 512x512 PtSi-Camera (Ueno et al. 1992). The plate scale was 4.″6 x 6.″0/pixel and the total field of view was 40.′2 x 52.′3. The system was attache作者: EVICT 時間: 2025-3-27 01:58 作者: 怎樣才咆哮 時間: 2025-3-27 07:45
Erika Fernández-Gómez,Beatriz Feijoo galaxies. Tidal dwarfs are found far from the interacting parent galaxies, associated with massive clouds of atomic hydrogen located at the tip of long tidal tails. These newly formed galaxies are among the best cases for the study of galaxy formation in the nearby Universe.作者: 漂白 時間: 2025-3-27 09:37
Manukonda Rabindranath,Aradhana Kumari Singhr to accretion and the triggering of star formation, show distinct HI signatures. Interactions and mergers in the recent past can also be recognized in the HI structure and kinematics. Recent 21cm line surveys of large samples of galaxies indicate that at least one out of every four galaxies shows s作者: Accomplish 時間: 2025-3-27 14:38 作者: corporate 時間: 2025-3-27 20:29
The Changing Face of Capitalism,s during an encounter, and the percentage of HI in the tails increases with the merging stage. However, the opposite is true for the molecular gas, which is observed highly concentrated towards the nuclei of interacting galaxies, amounting to a significant fraction of the dynamical mass. Statistical作者: 設(shè)施 時間: 2025-3-28 01:58
https://doi.org/10.1007/978-94-011-4665-4Galaxy; Universe; active galactic nuclei; astronomy作者: bromide 時間: 2025-3-28 04:10 作者: 天空 時間: 2025-3-28 07:54 作者: 吹牛需要藝術(shù) 時間: 2025-3-28 14:26 作者: Ceramic 時間: 2025-3-28 15:01 作者: MOTIF 時間: 2025-3-28 21:28
Adverse Drug Events to Biomedicineshe observed ellipticities (Shawl & White 1987) are ≥ 0.1 within ～ 2.. By a series of numerical experiments, we study whether or not tidal force from the Galactic disk can produce the observed ellipticities in such an inner region (Shimada 1996)作者: 不發(fā)音 時間: 2025-3-29 01:51 作者: 難取悅 時間: 2025-3-29 03:50
The Nature and Fate of the Sagittarius Dwarf Galaxy,d into the Milky Way. This unique event allows the physics of galactic merging to be probed in unprecedented detail, and may shed light on the hypothesized population of primordial galaxies that merged to form the Milky Way.作者: 刺激 時間: 2025-3-29 08:58
A Search for Moving Groups in the Galactic Halo,in this database. Although the sampled volume is small, the high quality of the astrometry makes this search interesting. No moving groups are detected, but limits in the velocity and number of members of possible non-detected groups are given.作者: alabaster 時間: 2025-3-29 12:33
Constraints on Interactions and Mergers from Dsph Galaxies and Globular Clusters,arf spheroidal (dSph) galaxy. Past mergers with dwarf galaxies may have contributed significantly to the Galactic halo and possibly to the thick disk. The properties of Local Group dSphs and halo globular clusters impose constraints on the merger history of the Milky Way.作者: 母豬 時間: 2025-3-29 19:36
The Magellanic Stream Revisited,s in accordance with the Keplerian law at the distance of 50 kpc, while others have come to consider that the rotation curve of the Milky Way, essentially stays flat or is still increasing at the distance of the Magellanic Clouds and the Magellanic Stream.作者: 可憎 時間: 2025-3-29 23:43 作者: 蒼白 時間: 2025-3-30 03:34
Tidal Dwarf Galaxies, galaxies. Tidal dwarfs are found far from the interacting parent galaxies, associated with massive clouds of atomic hydrogen located at the tip of long tidal tails. These newly formed galaxies are among the best cases for the study of galaxy formation in the nearby Universe.作者: CHARM 時間: 2025-3-30 04:55 作者: 刺穿 時間: 2025-3-30 08:12 作者: FANG 時間: 2025-3-30 13:18
https://doi.org/10.1007/978-3-031-08801-8We have investigated 4 Shapley constellations (1996, ., ., 40) to define the associated stellar complexes and their properties. From observed star counts and recent spectral classification we derive an age estimate and the upper mass limit of individual stars in these regions.作者: capsule 時間: 2025-3-30 18:09
Total Mass and Luminosity of Star Forming Regions in the Lmc: the Predicted Infrared Fluxes,We have investigated 4 Shapley constellations (1996, ., ., 40) to define the associated stellar complexes and their properties. From observed star counts and recent spectral classification we derive an age estimate and the upper mass limit of individual stars in these regions.作者: intimate 時間: 2025-3-30 22:58
Are the Bulge C-Stars Related to the Sagittarius Dwarf Galaxy?,n stars are in that case not metal-rich as previously thought, but they have a metallicity comparable to the LMC, with an age between 0.1–1 Gyr. A significant fraction of the carbon stars still have luminosities fainter than the lower LMC limit of. A similar trend is present among carbon stars found作者: 疏忽 時間: 2025-3-31 01:21
The High-Velocity Clouds: Galactic or Intergalactic?, stellar metal lines. Our distance bracket 4 < . < 11 kpc places Complex A in the Galactic Halo, at 2.5 < . < 7.5 kpc above the plane; a distance similar to Local Group galaxies is excluded. The HI mass implied lies between 0.15 and 1.2 times 10... Our result precludes local origins for this HVC. It作者: 使增至最大 時間: 2025-3-31 08:39
A Near Infrared Survey of the LMC,distributions of RSG, luminous giants and CO line flux are spatially different from each other. This supports the idea that the position of the active star forming region has changed during the past 10. years. The detected sources are cross-identified with the . Point Source Catalog. Sixty-two of 68作者: 畢業(yè)典禮 時間: 2025-3-31 11:59
Common Food Additives and Spices in Thailandn stars are in that case not metal-rich as previously thought, but they have a metallicity comparable to the LMC, with an age between 0.1–1 Gyr. A significant fraction of the carbon stars still have luminosities fainter than the lower LMC limit of. A similar trend is present among carbon stars found作者: CORE 時間: 2025-3-31 13:36
https://doi.org/10.1007/978-1-4302-3829-4 stellar metal lines. Our distance bracket 4 < . < 11 kpc places Complex A in the Galactic Halo, at 2.5 < . < 7.5 kpc above the plane; a distance similar to Local Group galaxies is excluded. The HI mass implied lies between 0.15 and 1.2 times 10... Our result precludes local origins for this HVC. It作者: HACK 時間: 2025-3-31 20:44 作者: 箴言 時間: 2025-3-31 22:10 作者: 擦掉 時間: 2025-4-1 02:49
https://doi.org/10.1007/978-3-0348-5722-2cimetric radio telescope in the velocity range of -529 to 1826 kms. with considerably better sensitivity (2–4 mJy rms.) than previous surveys. Half the objects observed are irregular dwarfs, expected to be H I-rich and detectable at Nan?ay if at the distance of the M81 group (4 Mpc).作者: 神圣將軍 時間: 2025-4-1 08:59 作者: GLIDE 時間: 2025-4-1 10:48
