標(biāo)題: Titlebook: Galactic Bulges; Eija Laurikainen,Reynier Peletier,Dimitri Gadotti Book 2016 Springer International Publishing Switzerland 2016 Dark Matte [打印本頁] 作者: Impacted 時(shí)間: 2025-3-21 16:15
書目名稱Galactic Bulges影響因子(影響力)
書目名稱Galactic Bulges影響因子(影響力)學(xué)科排名
書目名稱Galactic Bulges網(wǎng)絡(luò)公開度
書目名稱Galactic Bulges網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Galactic Bulges被引頻次
書目名稱Galactic Bulges被引頻次學(xué)科排名
書目名稱Galactic Bulges年度引用
書目名稱Galactic Bulges年度引用學(xué)科排名
書目名稱Galactic Bulges讀者反饋
書目名稱Galactic Bulges讀者反饋學(xué)科排名
作者: institute 時(shí)間: 2025-3-21 20:40 作者: 淘氣 時(shí)間: 2025-3-22 02:06 作者: Progesterone 時(shí)間: 2025-3-22 05:07 作者: LEVY 時(shí)間: 2025-3-22 10:55 作者: 察覺 時(shí)間: 2025-3-22 15:39 作者: 察覺 時(shí)間: 2025-3-22 20:06
A Universal Kinematic Scaling Relation and Galaxy Bulgesused fundamental plane in certain contexts. We then examine whether bulges separately satisfy the FM relation and discuss what the success or failure of such a match implies for the nature of classical- and pseudo-bulges. On the basis of this preliminary analysis we suggest that while classical bulg作者: 手銬 時(shí)間: 2025-3-22 22:01 作者: 按等級 時(shí)間: 2025-3-23 02:37
Theoretical Models of the Galactic Bulge witnessed a gradual paradigm shift in the formation and evolution of the Galactic bulge. Bulges were commonly believed to form in the dynamical violence of galaxy mergers. However, it has become increasingly clear that the main body of the Milky Way bulge is not a classical bulge made by previous m作者: graphy 時(shí)間: 2025-3-23 07:37
Galaxy Bulges and Their Massive Black Holes: A Reviewnce of massive black holes at the centers of galaxies. It then presents the historical development of the near-linear (black hole)–(host spheroid) mass relation, before explaining why this has recently been dramatically revised. Past disagreement over the slope of the (black hole)–(velocity dispersi作者: 駁船 時(shí)間: 2025-3-23 11:47 作者: seruting 時(shí)間: 2025-3-23 15:00
Bulge Growth Through Disc Instabilities in High-Redshift Galaxiesave long been studied in the low-redshift nearby Universe. There it has long been probed observationally, in particular through peanut-shaped bulges (Chap.?.). This secular growth of bulges in modern disc galaxies is driven by weak, non-axisymmetric instabilities: it mostly produces pseudobulges at 作者: infinite 時(shí)間: 2025-3-23 18:12 作者: hysterectomy 時(shí)間: 2025-3-23 22:45
Observed Properties of Boxy/Peanut/Barlens Bulgesn), or stellar populations (old), are similar to those observed in the Milky Way. Cool central discs are often embedded in the B/P/barlens bulges. Barred galaxies contain also dynamically hot classical bulges, but it is not yet clear to what extent they are really dynamically distinct structure comp作者: cumber 時(shí)間: 2025-3-24 05:38
The Milky Way Bulge: Observed Properties and a Comparison to External Galaxieserstand their origin. The investigation of both detailed and global properties of the bulge now provide us with the opportunity to characterize the bulge as observed in models, and to place the mixed component bulge scenario in the general context of external galaxies. When writing this review, we c作者: Ondines-curse 時(shí)間: 2025-3-24 07:46 作者: Misgiving 時(shí)間: 2025-3-24 12:53
Bulge Formation via Mergers in Cosmological Simulationsies. After reviewing the results of relevant research that has been published to date, we use cosmological simulations to explore the ability of feedback to reduce or even prevent bulge growth during mergers. In dwarf galaxies, mergers actually reduce the central concentration of galaxies as the ind作者: d-limonene 時(shí)間: 2025-3-24 18:22 作者: palpitate 時(shí)間: 2025-3-24 20:31 作者: Melanoma 時(shí)間: 2025-3-25 01:00 作者: GIBE 時(shí)間: 2025-3-25 05:19
Advances in Elastomers and Rubber Elasticityn), or stellar populations (old), are similar to those observed in the Milky Way. Cool central discs are often embedded in the B/P/barlens bulges. Barred galaxies contain also dynamically hot classical bulges, but it is not yet clear to what extent they are really dynamically distinct structure comp作者: 致敬 時(shí)間: 2025-3-25 08:48 作者: 拋棄的貨物 時(shí)間: 2025-3-25 14:20 作者: URN 時(shí)間: 2025-3-25 17:55
Participatory and Action Research Methodsies. After reviewing the results of relevant research that has been published to date, we use cosmological simulations to explore the ability of feedback to reduce or even prevent bulge growth during mergers. In dwarf galaxies, mergers actually reduce the central concentration of galaxies as the ind作者: compassion 時(shí)間: 2025-3-25 22:49
https://doi.org/10.1007/978-981-10-4041-2t instability drive disc evolution and bulge growth through various mechanisms on short timescales. The giant clumps can migrate inward and coalesce into the bulge in a few 10.?years. The instability in the very turbulent media drives intense gas inflows toward the bulge and nuclear region. Thick di作者: 顯而易見 時(shí)間: 2025-3-26 03:42 作者: 氣候 時(shí)間: 2025-3-26 05:38
The Intrinsic Shape of Galaxy Bulgesaxy discs is then presented in a historical context, in order to place the role that the 3D structure of bulges play in the broader picture of galaxy evolution. Our current view on the 3D shape of the Milky Way bulge and future prospects in the field are also depicted.作者: callous 時(shí)間: 2025-3-26 11:19
0067-0057 le of the various types of bulges during the mass build-up oThis book consists of invited reviews on Galactic Bulges written by experts in the field. A central point of the book is that, while in the standard picture of galaxy formation a significant amount of the baryonic mass is expected to reside作者: PLE 時(shí)間: 2025-3-26 13:58
Advances in Criterion-Referenced Measurementncluding morphology, structural properties, star formation, gas content & stellar population, and kinematics. We conclude by summarizing those properties that isolate pseudobulges from classical bulges. Our intention is to describe a practical, easy to use, list of criteria for identifying bulge types.作者: plasma-cells 時(shí)間: 2025-3-26 19:44
Gerald A. Walker (Assistant Editor)verview of how our perspective on galactic bulges has changed over the years. While it is mainly focused on aspects related to the dynamical state of their stars, there will be natural connections to other properties (e.g. morphology, stellar populations) discussed in other reviews in this volume.作者: 整潔漂亮 時(shí)間: 2025-3-26 21:50 作者: 錫箔紙 時(shí)間: 2025-3-27 01:39
An Observational Guide to Identifying Pseudobulges and Classical Bulges in Disc Galaxiesncluding morphology, structural properties, star formation, gas content & stellar population, and kinematics. We conclude by summarizing those properties that isolate pseudobulges from classical bulges. Our intention is to describe a practical, easy to use, list of criteria for identifying bulge types.作者: CRUDE 時(shí)間: 2025-3-27 07:19 作者: Respond 時(shí)間: 2025-3-27 12:42 作者: Omnipotent 時(shí)間: 2025-3-27 14:02
Saccharide based contrast agentsgenerically as “bulges”. That term finally won out over its more unwieldy competitors such as the “amorphous central region”, the “unresolved nuclear region” or the highly ambiguous term “central nucleus”.作者: 不透氣 時(shí)間: 2025-3-27 21:38 作者: 性行為放縱者 時(shí)間: 2025-3-28 00:43
Advances in Endophytic Research the scaling relation and so probably consist of an unrepresentative subset of disc stars. This is currently not a unique explanation of the results, but the use of kinematic scaling relations with larger samples, done in a more systematic manner, could lead to a more definitive resolution on the nature of bulges.作者: Mendacious 時(shí)間: 2025-3-28 05:20 作者: 四指套 時(shí)間: 2025-3-28 08:37
Bulges: Seen from a Philosophically-Informed Historical Perspective,generically as “bulges”. That term finally won out over its more unwieldy competitors such as the “amorphous central region”, the “unresolved nuclear region” or the highly ambiguous term “central nucleus”.作者: lobster 時(shí)間: 2025-3-28 10:58
Nuclear Star Clusters and Bulges 100?Myr. Therefore star formation must be happening either directly in the nuclear star cluster or in its vicinity. The secular processes that fuel the formation of pseudobulges very likely also contribute to nuclear star cluster growth.作者: vitreous-humor 時(shí)間: 2025-3-28 18:13
A Universal Kinematic Scaling Relation and Galaxy Bulges the scaling relation and so probably consist of an unrepresentative subset of disc stars. This is currently not a unique explanation of the results, but the use of kinematic scaling relations with larger samples, done in a more systematic manner, could lead to a more definitive resolution on the nature of bulges.作者: 天空 時(shí)間: 2025-3-28 20:07
Galaxy Bulges and Their Massive Black Holes: A Reviewor the fundamental connection between massive black holes and their host galaxies continues, the competing array of additional black hole mass scaling relations for samples of predominantly inactive galaxies are presented.作者: meditation 時(shí)間: 2025-3-29 01:17 作者: lymphoma 時(shí)間: 2025-3-29 04:21
Encapsulants for Electronic Packaging,This chapter summarizes our current understanding of the stellar population properties of bulges and outlines important future research directions.作者: nonplus 時(shí)間: 2025-3-29 07:20 作者: 擁護(hù)者 時(shí)間: 2025-3-29 12:42 作者: FLACK 時(shí)間: 2025-3-29 17:00
Saccharide based contrast agentsonal astronomers knew, or even cared. We trace the early and quite casual usage of the term (and its competitors) and then follow the later and gradually more strict adoption of the term “bulge”, needed to call out a major component of galaxy morphology. In the specific context of the Milky Way “The
