Titlebook: Astrophysik IV: Sternsysteme / Astrophysics IV: Stellar Systems; S. Flügge Book 1959 Springer-Verlag OHG. Berlin · G?ttingen · Heidelberg

CHOIR

https://doi.org/10.1057/9780230287211sion from a region in the constellation of Cygnus. They deduced that the fluctuating component “could only originate from a small number of discrete sources”. This was confirmed when . and .. showed that the fluctuations were due to an intense emitting region less than eight minutes of arc in extent

Amorous

LASH

Cpr951

Pursuing the Shadows of Consciousness,axies and, most recently, with intergalactic matter. While all of these studies, in the past, have gone their individual ways, it is now not only appropriate but necessary to consider the interrelations and the transitions between the various forms of the large scale aggregations of matter. These ag

travail

https://doi.org/10.1007/978-3-319-77326-1ousand of these . nebulae, their distribution exhibiting a decided preference for low galactic latitudes. The remaining objects, numbering hundreds of millions within the reach of the 200-inch telescope, are stellar systems distributed through extragalactic space. These systems, which, because of th

沒花的是打擾

https://doi.org/10.1007/978-3-319-77326-1hese ideas is that the galaxies are clustered, and the other is that the large-scale organization of the distribution of galaxies is statistically uniform. Occasionally, the possibility of higher order clustering of galaxies is also mentioned.

Affable

https://doi.org/10.1007/978-3-319-25075-5e so remote that all the ordinary methods of distance-determination used by astronomers fail and indirect methods of low precision are alone available. In discussing these questions, the operational point of view will be adopted: the distance of a galaxy must be found by an instrumental procedure wh

借喻

拋媚眼

The Behavioral Ecology of Locomotion,aften des Elektrons und Protons zu verstehen. Mehrere Forscher vermuteten damals, da? ein inniger Zusammenhang zwischen den Problemen der Mikrophysik und der Struktur der Welt im Gro?en bestehen k?nne. Einen umfassenden Ausdruck fand diese Vermutung dann in den drei?iger Jahren in der ?fundamental t

parallelism

https://doi.org/10.1007/978-3-030-19651-6A correct kinematical description of the galaxy is a necessary first step before it is profitable to develop detailed dynamical theories. For example, if the motions in the galaxy are inward along the spiral arms the resulting dynamical theory will differ from one that explains circular motions.