Titlebook: Island Universes; Structure and Evolut R. S. DE JONG Conference proceedings 2007 Springer Science+Business Media B.V. 2007 Accretion.Bulge.

動詞

書目名稱Island Universes影響因子(影響力)




書目名稱Island Universes影響因子(影響力)學科排名




書目名稱Island Universes網(wǎng)絡公開度




書目名稱Island Universes網(wǎng)絡公開度學科排名




書目名稱Island Universes被引頻次




書目名稱Island Universes被引頻次學科排名




書目名稱Island Universes年度引用




書目名稱Island Universes年度引用學科排名




書目名稱Island Universes讀者反饋




書目名稱Island Universes讀者反饋學科排名

Notify

Exposure

FEEDING THE NUCLEAR STARBURST IN NGC6946de a detailed test for models of nuclear gas spirals inside the inner Lindblad resonance as a possible funneling mechanism towards galactic nuclei, and will be used to constrain the efficiency of nuclear star formation in NGC 6946.

deciduous

bonnet

HALO MASS PROFILES OF LOW SURFACE BRIGHTNESS GALAXIES an improved analysis method that shows that only a small minority of LSB rotation curves is possibly consistent with CDM simulations. The large majority prefer semi-constant kpc-sized mass-density cores.

顧客

THE CONTRIBUTION OF LSB GALAXIES TO THE LOCAL GALAXY NUMBER DENSITYl surveys and point out the in-fluence of different search algorithms and size estimation methods at the number density. The contribution of LSB galaxies to the local galaxy number density is about 30% and thus not negligible.

Immunization

1570-6591 ft observations, theory and observations.This book contains an up-to-date review of the structure and evolution of disk galaxies from both the observational and theoretical point of view. The book is the proceedings of the "Island Universes" conference held at the island of Terschelling, The Netherl

irradicable

EXTRAGALACTIC THICK DISKSmore metal-poor than those surrounding massive disk galaxies. Given the strong evidence that thick disks are fossils from an early epoch of merging, these trends place tight constraints on the early assembly of disk galaxies.

拋射物

THE THIN AND THICK DISKS OF THE GALAXY: DIFFERENCES IN EVOLUTIONre smooth and quiet than the star formation history of the thick disk of our Galaxy. Gas infall plays an important role in creating relative abundance differences between the thin and thick disk — the inflow rate is more intense for the thick disk.

Ganglion

COUNTERROTATING CORE IN THE LMC: ACCRETION AND/OR MERGER?s in the inner LMC, with one coun-terrotating. This two disk model is found to match the Hi velocities as well. The presence of a counter-rotating core could be due to internal (secondary bar) / external (gas accretion) origin.