標題: Titlebook: Environment and the Formation of Galaxies: 30 years later; Proceedings of Sympo Ignacio Ferreras,Anna Pasquali Conference proceedings 2011 [打印本頁] 作者: Philanthropist 時間: 2025-3-21 16:56
書目名稱Environment and the Formation of Galaxies: 30 years later影響因子(影響力)
書目名稱Environment and the Formation of Galaxies: 30 years later影響因子(影響力)學(xué)科排名
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書目名稱Environment and the Formation of Galaxies: 30 years later網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Environment and the Formation of Galaxies: 30 years later被引頻次
書目名稱Environment and the Formation of Galaxies: 30 years later被引頻次學(xué)科排名
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書目名稱Environment and the Formation of Galaxies: 30 years later年度引用學(xué)科排名
書目名稱Environment and the Formation of Galaxies: 30 years later讀者反饋
書目名稱Environment and the Formation of Galaxies: 30 years later讀者反饋學(xué)科排名
作者: jeopardize 時間: 2025-3-21 23:28
The Cosmic Mass Density Field Reconstruction from the SDSS Group Catalog,roduced by [Wang et al., MNRAS 394, 398 (2009)]. The method uses the mass distribution in and around dark matter structures computed from cosmological simulations to map the cosmic mass distribution. This approach enables us to make reconstructions of the density field avoiding the use of arbitrary 作者: Carcinoma 時間: 2025-3-22 02:18
The Void Galaxy Survey,entified voids in the SDSS redshift survey on the basis of a unique geometric technique, with no a prior selection of intrinsic properties of the void galaxies. The project intends to study in detail the gas content, star formation history and stellar content, as well as kinematics and dynamics of v作者: Malfunction 時間: 2025-3-22 08:38 作者: engrave 時間: 2025-3-22 08:47
The Dependence of Low Redshift Galaxy Properties on Environment,, group-centric radius, and the distinction between centrals and satellites; examined galaxy properties include star formation rate, colour, AGN fraction, age, metallicity and concentration. In general, satellite galaxies diverge more markedly from their central counterparts if they reside in more m作者: AVOID 時間: 2025-3-22 15:44 作者: AVOID 時間: 2025-3-22 20:07
The Fossil Candidate RX J1548.9+0851,ynamical friction as the driving process leads to the coalescence of individual galaxies in ordinary poor groups, leaving behind nothing more than a central, massive elliptical galaxy supposed to contain the merger history of the whole group. Due to longer merging timescales for less-massive galaxie作者: GROSS 時間: 2025-3-23 00:30
The Environments of Luminous Infrared Galaxies,arks an important luminosity point among IR galaxies - the large scale density of environment around LIRGs correlates strongly with their SFR above this value at a fixed stellar mass. On the other hand there is no clear correlation between stellar mass and density at constant SFR. No matter what the作者: 智力高 時間: 2025-3-23 01:26
,UV–IR Luminosity Functions and Stellar Mass Functions of Galaxies in the Shapley Supercluster Core, z??=?0.048, in order to investigate how the dense environment affects the galaxy properties, such as star formation (SF) or stellar mass. We find that, while the faint-end slope of optical and NIR LFs steepens with decreasing density, no environment effect is found in the slope of the SMFs. This su作者: 增減字母法 時間: 2025-3-23 09:22
Component Luminosity Functions of Galaxy Pairs in the MGC,ging systems (Casteels and Patton 2011). Using mock catalogues, the effect of imposing a fixed magnitude separation (.) between galaxy pairs (to isolate major mergers) is explored and we find that imposing a . introduces a selection bias which must be corrected for when comparing with field LFs. Our作者: Pedagogy 時間: 2025-3-23 10:16 作者: CLAN 時間: 2025-3-23 17:15
The Symbiotic Relationship Between the Evolution of Galaxy Groups and Their Resident Galaxies,ediate environment rather than in larger clusters. We report on observational and analytical work that shows how the evolution of the group environment influences the evolution of the resident galaxies and how feedback resulting from the evolution of individual galaxies influences their larger envir作者: 遺傳 時間: 2025-3-23 18:09 作者: 黑豹 時間: 2025-3-24 01:59
The Fundamental Plane of Early-Type Galaxies: Environmental Dependence from , Through ,, (ETGs) in the optical (griz) and Near-Infrared (YJHK) wavebands. The intercept “.” of the FP decreases from high- to low-density regions, implying that galaxies at low density have on average lower mass-to-light ratios than their high-density counterparts. Since the variation of “.” is the same at 作者: 固執(zhí)點好 時間: 2025-3-24 02:44
,On Galaxy Mass–Radius Relationship,on follows about the observed relationship between stellar mass and effective radius, ..???.., for early type galaxies (ETGs). The key of this correlation lies in the deep link which has to exist between cosmology and the existence of the?FP. The general strategy consists in using the two-component 作者: 字的誤用 時間: 2025-3-24 08:29 作者: 古代 時間: 2025-3-24 13:21 作者: Yag-Capsulotomy 時間: 2025-3-24 17:44 作者: 骯臟 時間: 2025-3-24 22:27
Wundballistik -- Grundlagen und AnwendungenUsing data from our Parkes and ATCA .?survey of six groups analogous to the Local Group, we find that the .?mass function and velocity distribution function for loose groups are the same as those for the Local Group. Both mass functions confirm that the “missing satellite” problem exists in other galaxy groups.作者: 玷污 時間: 2025-3-25 02:15 作者: PANG 時間: 2025-3-25 04:12 作者: 消息靈通 時間: 2025-3-25 08:41
Astrophysics and Space Science Proceedingshttp://image.papertrans.cn/e/image/312476.jpg作者: ANTE 時間: 2025-3-25 15:17
https://doi.org/10.1007/978-3-642-20285-8AGN feedback; Clusters of Galaxies; Cosmic Voids; Galactic Environment; Galactic Halos; Galaxy Formation 作者: 裂隙 時間: 2025-3-25 17:09 作者: 蹣跚 時間: 2025-3-25 23:56
Environment and the Formation of Galaxies: 30 years later978-3-642-20285-8Series ISSN 1570-6591 Series E-ISSN 1570-6605 作者: 粗糙 時間: 2025-3-26 02:17 作者: concentrate 時間: 2025-3-26 04:42 作者: Negligible 時間: 2025-3-26 09:34
https://doi.org/10.1007/978-3-031-43710-6entified voids in the SDSS redshift survey on the basis of a unique geometric technique, with no a prior selection of intrinsic properties of the void galaxies. The project intends to study in detail the gas content, star formation history and stellar content, as well as kinematics and dynamics of v作者: Gobble 時間: 2025-3-26 15:47
Progress Testing in Written Assessment,warfs. We compiled a sample of about one hundred dwarfs with M. in the range –12to –18 mag, falling within the nearby Lynx-Cancer void. The goal is to study their evolutionary parameters – gas metallicity and gas mass-fraction, and to address the epoch of the first substantial episode of Star Format作者: 輕彈 時間: 2025-3-26 20:12 作者: 變色龍 時間: 2025-3-26 21:23
https://doi.org/10.1007/978-3-662-46084-9alogues extracted from the Millennium simulation to study the potential systematics that might affect the overall distribution of the identified systems. We train on these mock catalogues the adopted group-finding technique (the Voronoi-Delaunay Method, VDM), to recover in an unbiased way the redshi作者: 嘴唇可修剪 時間: 2025-3-27 04:37 作者: 感染 時間: 2025-3-27 08:04 作者: FOR 時間: 2025-3-27 10:08 作者: AGOG 時間: 2025-3-27 14:01
https://doi.org/10.1007/978-3-662-64859-9ging systems (Casteels and Patton 2011). Using mock catalogues, the effect of imposing a fixed magnitude separation (.) between galaxy pairs (to isolate major mergers) is explored and we find that imposing a . introduces a selection bias which must be corrected for when comparing with field LFs. Our作者: 泥沼 時間: 2025-3-27 18:53 作者: Blazon 時間: 2025-3-28 01:09 作者: Contend 時間: 2025-3-28 02:06
https://doi.org/10.1007/978-3-662-58697-6 the origin of this effect is not well known to date, and quantitative studies are rare. Here, we present the first statistical investigation of a sample of 76 H. discs using the WHISP survey. We perform a Fourier analysis to study the morphological lopsidedness. This allows to trace the degree of a作者: guzzle 時間: 2025-3-28 09:41
https://doi.org/10.1007/978-3-642-73004-7 (ETGs) in the optical (griz) and Near-Infrared (YJHK) wavebands. The intercept “.” of the FP decreases from high- to low-density regions, implying that galaxies at low density have on average lower mass-to-light ratios than their high-density counterparts. Since the variation of “.” is the same at 作者: reject 時間: 2025-3-28 10:33 作者: Arbitrary 時間: 2025-3-28 16:51 作者: overture 時間: 2025-3-28 21:43 作者: chalice 時間: 2025-3-29 01:52
,Wundt’s Idea of a Scientific Philosophy,9, 2562 (2005)]. Using EURO-VO tools we obtained multiwavelength data, we built spectral energy distributions, and undertook a thorough analysis to ascertain: the frequency of AGN among these galaxies, the degree of star formation and intrinsic extinction. We aim at verifying whether there are bulge作者: SSRIS 時間: 2025-3-29 04:55
1570-6591 e environmental dependence of galaxy properties at z ≥ 1 and the implementation of environmental effects in cosmological models of galaxy formation and evolution..This book presents the edited proceedings of this stimulating meeting..978-3-642-26995-0978-3-642-20285-8Series ISSN 1570-6591 Series E-ISSN 1570-6605 作者: Tailor 時間: 2025-3-29 07:34
Of Women, Writing, and Recognition, galaxy formation, passed down by the hierarchical growth of structure. In fact, it seems increasingly likely that the more fundamental correlation of galaxy morphology is with galaxy mass, and that the morphology–density relation is basically an expression of the prevalence of more massive galaxies作者: 逢迎春日 時間: 2025-3-29 11:25
https://doi.org/10.1007/978-3-662-10980-9he infrared (IR) LFs suggests that the bulk of the star-forming galaxies that make up the observed cluster IR LF have been recently accreted from the field and have yet to have their SF activity significantly affected by the cluster environment.作者: 哄騙 時間: 2025-3-29 17:01 作者: ULCER 時間: 2025-3-29 20:07 作者: absorbed 時間: 2025-3-30 01:26
Environment and the Formation of Galaxies: 30 years laterProceedings of Sympo作者: Custodian 時間: 2025-3-30 07:18 作者: Juvenile 時間: 2025-3-30 10:04
,UV–IR Luminosity Functions and Stellar Mass Functions of Galaxies in the Shapley Supercluster Core,he infrared (IR) LFs suggests that the bulk of the star-forming galaxies that make up the observed cluster IR LF have been recently accreted from the field and have yet to have their SF activity significantly affected by the cluster environment.作者: atopic-rhinitis 時間: 2025-3-30 13:29
And the Winner Is: Galaxy Mass,literature that galaxy mass is the major driver of galaxy formation. Even the morphology–density relationship may actually be mass-driven, as the consequence of an environment dependent characteristic galaxy mass coupled with the fact that late-type galaxy morphologies are more prevalent in low-mass作者: 清洗 時間: 2025-3-30 17:30 作者: recession 時間: 2025-3-30 23:35 作者: Firefly 時間: 2025-3-31 03:04
Lopsidedness in WHISP Galaxies,ple of 76 H. discs using the WHISP survey. We perform a Fourier analysis to study the morphological lopsidedness. This allows to trace the degree of asymmetry with radius. We further investigate the dependence on, e.g., the morphological type and environment.作者: Recessive 時間: 2025-3-31 07:45
AGN Feedback and Quenching of Star Formation: A Multiwavelength Approach with the EURO-VO,certain: the frequency of AGN among these galaxies, the degree of star formation and intrinsic extinction. We aim at verifying whether there are bulgeless quenched galaxies hosting SMBHs in order to test the AGN feedback paradigm.作者: Expressly 時間: 2025-3-31 11:01 作者: Encoding 時間: 2025-3-31 14:46 作者: dagger 時間: 2025-3-31 19:17 作者: 現(xiàn)暈光 時間: 2025-3-31 23:57
Energien, Kr?fte und das Anderswo the “newcomers” in the cluster. Most Hercules SF galaxies follow well defined mass-metallicity and luminosity-metallicity sequences; nevertheless significant outliers to these relations have been identified, illustrating how environmental effects can provide a physical source of dispersion in these fundamental relations.作者: EWER 時間: 2025-4-1 02:24 作者: 感情 時間: 2025-4-1 07:42
Metallicities of Galaxies in the Lynx-Cancer Void,ion. Here we present and discuss the results of O/H measurements in 38 void galaxies, among which several of the most metal-poor galaxies are found with an oxygen abundance of 12?+?log(O∕H)?=?7.?12–7.3?dex.作者: uveitis 時間: 2025-4-1 12:51
The Fossil Candidate RX J1548.9+0851,s, a surrounding faint-galaxy population and an extended X-ray halo similar to that found in ordinary poor groups, is expected. Multi-object spectroscopy with VIMOS has been performed to study the faint galaxy population of the fossil candidate RX J1548.9?+?0851.作者: violate 時間: 2025-4-1 15:13 作者: 上腭 時間: 2025-4-1 20:25
