Results 61 to 70 of about 173,443 (344)
Prepositive Synergistic Bulge Design for Improving Aerodynamic Performance of Submerged Inlet
Aerospace, 2023 A submerged inlet has good stealth characteristics and a low external drag, but it also has the disadvantage of low internal flow efficiency. In view of this, a new efficiency enhancement method based on the prepositive synergistic bulge of the inlet’s ...
Xuan Bai, Baigang Mi
doaj +1 more source
The X-shaped Bulge of the Milky Way revealed by WISE [PDF]
, 2016 The Milky Way bulge has a boxy/peanut morphology and an X-shaped structure. This X-shape has been revealed by the `split in the red clump' from star counts along the line of sight toward the bulge, measured from photometric surveys. This boxy, X-shaped bulge morphology is not unique to the Milky Way and such bulges are observed in other barred spiral ...
arxiv +1 more source
, 2000 We model the evolution of the galactic bulge and of the bulges of a selected sample of external spiral galaxies, via the multiphase multizone evolution model. We address a few questions concerning the role of the bulges within galactic evolution schemes and the properties of bulge stellar populations.
Molla, M., Ferrini, F., Gozzi, G.
openaire +2 more sources
Central Bulge Ferrite Core for Efficient Wireless Power Transfer
Energies, 2021 To improve the efficiency of the wireless power transfer (WPT) system without increasing the system size, a central bulge ferrite core with a novel configuration is proposed.
Huabo Xu, Huihui Song, Rui Hou
doaj +1 more source
Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars. II. Ages, metallicities, detailed elemental abundances, and connections to the Galactic thick disc [PDF]
, 2010 The Bulge is the least understood major stellar population of the Milky Way. Most of what we know about the formation and evolution of the Bulge comes from bright giant stars.
A. Gal-Yam +86 more
core +2 more sources
Resolved properties of classical bulge and pseudo-bulge galaxies [PDF]
arXiv, 2023 We compare properties of classical and pseudo-bulges and properties of their hosting galaxies selected from the MaNGA survey. Bulge types are identified based on the S$\mathrm{\acute{e}}$rsic index n of bulge component and the position of bulges on the Kormandy diagram.
arxiv
Another bar in the Bulge [PDF]
Astronomy & Astrophysics, 2001 A map of the projected density of the old stellar population of the Galactic Bulge region is reconstructed using 2MASS data. By making a combination of the H and K photometric bands, it is possible to overcome the effect of reddening, and thus penetrate the inner structure of the Galactic Bulge.
openaire +6 more sources
Thick disk and pseudobulge formation in a clump cluster
EPJ Web of Conferences, 2012 Bulges in spiral galaxies have been supposed to be classified into two types: classical bulges or pseudobulges. Classical bulges are thought to form by galactic merger with bursty star formation, whereas pseudobulges are suggested to form by secular ...
Inoue S.
doaj +1 more source
, 2013 We investigate the large scale metallicity distribution in the Galactic bulge, using a large spatial coverage, in order to constrain the bulge formation scenario.
Gonzalez, O. A. +5 more
core +1 more source
The Structure of Classical Bulges And Pseudobulges: The Link Between Pseudobulges And Sersic Index [PDF]
, 2008 In this paper we study the properties of pseudobulges (bulges that appear similar to disk galaxies) and classical bulges (bulges which appear similar to E-type galaxies) in bulge-disk decompositions. We show that the distribution of bulge Sersic indices is bimodal, and this bimodality correlates with the morphology of the bulge.
arxiv +1 more source