Titlebook: Extragalactic Astronomy and Cosmology; An Introduction Peter Schneider Textbook 20061st edition Springer-Verlag Berlin Heidelberg 2006 Cosm

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https://doi.org/10.1007/978-3-642-59264-5ich we are able to study astrophysical processes in detail. Therefore, our journey through extragalactic astronomy will begin in our home Galaxy, with which we first need to become familiar before we are ready to take off into the depths of the Universe. Knowing the properties of the Milky Way is in

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,überbetriebliche Informationsintegration,instead we will turn our attention to the space and time in which these objects are embedded. These considerations will then lead to a world model, the model of our cosmos. .This chapter will deal with aspects of homogeneous cosmology. As we will see, the Universe can, to first approximation, be con

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Von der “Arriflex” zum “Fly-away”is is thermal radiation since the emitting plasma in stellar atmospheres is basically in thermodynamical equilibrium. To a first approximation, the spectral properties of a star can be described by a Planck spectrum whose temperature depends on the stellar mass and the evolutionary state of the star

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Vorgehensweise der empirischen Untersuchung,he projection of bright galaxies on the sky (see Figs. 6.1 and 6.2). The Milky Way itself is a member of a group, called the Local Group (Sect. 6.1), which implies that we are living in a locally overdense region of the Universe.

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Information als Wettbewerbsfaktor,ption of a (spatially) homogeneous and isotropic Universe. Of course, the assumption of homogeneity is justified only on large scales because observations show us that our Universe is inhomogeneous on small scales – otherwise no galaxies or stars would exist.

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,Elektronische Marktpl?tze und Beschaffung,ies, and AGNs that we have gained in the other chapters, we are now ready to discuss the determination of the various cosmological parameters. In the course of this discussion, we will describe a number of methods, each of which is in itself useful for estimating cosmological parameters, and we will

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Informationsmanagement im MittelstandIn the final chapter of this book, we will dare to give an outlook for the fields of extragalactic astronomy and cosmology for the next few years from the perspective of 2006.