Milky Way Galaxy, large spiral system consisting of several hundred billionstars, one of which is theSun. It takes its name from the Milky Way, the irregularluminousband of stars and gas clouds that stretches across the sky as seen fromEarth. Although Earth lies well within the Milky Way Ga...
Studying the Milky Way used to be notoriously difficult. Astronomers sometimes compare the effort to attempting to describe the size and structure of a forest while being lost in the middle of it. From our position onEarth, we simply lack an overview. But two ground-breaking space telescopes l...
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For comparison, the Aquarius [234] and Via Lactea-II [257] simulations of Milky Way-mass halos contain nearly a billion particles within the virial radius of their respective halos. In order to interpret the VDF from these simulations, it is best to establish a point of comparison. With ...
We revisit the well known discrepancy between the observed number of Milky Way (MW) dwarf satellite companions and the predicted population of cold dark ma... SE Koposov,Y Jaiyul,R Hans-Walter,... - 《Astrophysical Journal》 被引量: 209发表: 2009年 The Local Group in comparison with othe...
“game” don’t understand it, I think a nova game were you make supernovas or something like that and a game with a black hole being able to put objects inside it to make it bigger lastly update size comparison make it like a black hole compared to the earth, by the way still a...
Bottom graph is a zoom on the area beyond 16 kpc which allows to see the excellent agreement of the GR expression (10) with measurements of the rotation speed of the Milky Way. Full size image Application to the precession of the galactic disks warp...
In Sect. 5, we use astrophysical data of the Milky Way (MW) and M31 galaxies to constrain the free parameters of the Yukawa model. Furthermore, in Sect. 6, we discuss results in light of the most recent findings in the literature. Finally, Sect. 7 is devoted to the conclusions and ...
Dust Grain Size Distributions and Extinction in the Milky Way, LMC, and SMC We construct size distributions for carbonaceous and silicate grain populations in different regions of the Milky Way, LMC, and SMC. The size distributions... JC Weingartner,BT Draine - 《Astrophysical Journal》 被引量...