Titlebook: Galactic Bulges; Eija Laurikainen,Reynier Peletier,Dimitri Gadotti Book 2016 Springer International Publishing Switzerland 2016 Dark Matte

GIBE

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

致敬

拋棄的貨物

URN

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

compassion

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

顯而易見

氣候

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.

callous

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

PLE

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.

plasma-cells

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.