Titlebook: Galaxies and their Masks; A Conference in Hono David L. Block,Kenneth C. Freeman,Ivanio Puerari Conference proceedings 2010 Springer Scienc

Tyler

書目名稱Galaxies and their Masks影響因子(影響力)




書目名稱Galaxies and their Masks影響因子(影響力)學(xué)科排名




書目名稱Galaxies and their Masks網(wǎng)絡(luò)公開度




書目名稱Galaxies and their Masks網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Galaxies and their Masks被引頻次




書目名稱Galaxies and their Masks被引頻次學(xué)科排名




書目名稱Galaxies and their Masks年度引用




書目名稱Galaxies and their Masks年度引用學(xué)科排名




書目名稱Galaxies and their Masks讀者反饋




書目名稱Galaxies and their Masks讀者反饋學(xué)科排名

Banquet

Kenneth Lyons Jones,H. Eugene Hoymeuch as rings, nuclear arms, nuclear bars, and asymmetries. We find a centrally peaked concentration in about 85% of the galaxies with typical size scales of about 0.5–1 kpc. This might be related to perturbations produced by recent interactions.

情節(jié)劇

飛行員

使虛弱

LEERY

Sonal,Sharmita Gupta,Yati Prabha,S. K. Sonillicity gradient, bars with null metallicity gradient, and galaxies with positive metallicity gradient. Regarding the bulge region we find that the ages and metallicities are younger and more metal rich, at a given ., than the bulges of unbarred galaxies. The bulges of the barred galaxies in our sam

LEERY

obeisance

組成

PHIL

The Large Magellanic Cloud: A Power Spectral Analysis of Spitzer Images,similar to the in-plane velocities at small scales. The motions are highly anisotropic at large scales,with in-plane velocities being much more important than vertical ones.In contrast, at small scales, the motions become more isotropic.