We analyze the resolved stellar populations of 473 massive star-forming galaxies at 0.7 {lt} z {lt} 1.5, with multi-wavelength broadband imaging from CANDE... S Wuyts,NM F?Rster Schreiber,EJ Nelson,... - 《Astrophysical Journal》 被引量: 60发表: 2013年 Multicultural Stories Preservice Tea...
As an analogy, consider the shape of our galaxy, the Milky Way. We can infer that it is a spiral based on maps of the stars in its spiral arms, but we cannot go outside the galaxy to see this spiral structure firsthand. However, with telescopes, we can see other spiral galaxies fro...
Twitter Google Share on Facebook Dictionary </>embed</> knot gnarl warp buckle contortion tortuousness tortuosity torsion distortion distorted... noun Synonyms for distorted shape nouna shape resulting from distortion Synonyms distortion Related Words ...
On the Nature of Soft X-ray Weak Quasi-Stellar Objects Galaxies: ActiveGalaxies: NucleiGalaxies: Quasars: GeneralX-Rays: GalaxiesRecent studies of QSOs with ROSAT suggest the existence of a significant population... WN Brandt,A Laor,BJ Wills - 《Astrophysical Journal》...
Whether theshapeof the cluster was the same on the left side as on the right side. 指的是星团右侧的形状和左侧的形状是不是一样。 来源于:听力OFFICIAL42 L3 You are talking about theshapeof the cluster though, not theshapeof the galaxies within the cluster. ...
Constraints on the Mass of Warm Dark Matter Particles and the Shape of the Linear Power Spectrum from the Lyα Forest High-resolution N-body simulations of cold dark matter (CDM) models predict that galaxies and clusters have cuspy halos with considerable substructure. Obs... VK Narayanan,DN ...
“This continuous cycle of accretion, recycling and outflows is referred to as the baryon cycle. Galaxies can be conceptualized as baryon processing engines, drawing gas from the intergalactic medium and converting some of it into stars. Stars, in turn, go supernova, producing heavier elements. ...
The Role of Stellar Halos in Understanding Galaxies The Milky Way’s stellar halo is the visible portion of what is more broadly called the galactic halo. This galactic halo is dominated by invisible dark matter, whose presence is only measurable through the gravity that it exerts. Every galaxy...
57% (583) of all 1028 galaxies in GOODS-Sshow a single component in the ACS/F850LP image. As WFC3/F160W images coveronly some part of GOODS-S and SXDS, 724/1028 and 2500/29835 sBzK galaxies inthe GOODS-S and SXDS have the WFC3 coverage. 86% (626) and 82% (2044) of thesB...
galaxies etc. can be fitted efficiently using a combination of these com-ponents. The results of these fits provide further insight in the compo-sition of the emitting material and the local physical conditions. In theframe of the future IR space missions (JWST, SPICA), this approachcan be...