Results 211 to 220 of about 1,645,813 (249)
A large, long-lived, slowly-expanding superbubble across the Perseus arm. [PDF]
Chen B +7 more
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The Physics of Galaxy Cluster Outskirts [PDF]
56 pages. Review paper.
Dominique Eckert +2 more
exaly +5 more sources
The physics of dissipational galaxy formation
A number of arguments lead one to consider the possibility that the first massive galaxies were formed after redshift 10. The formation of galaxies at small redshifts can only have occurred if the formation process was dissipative. This paper is concerned with one theory of dissipative galaxy formation: the theory which arises from the supposition that
James Binney
exaly +2 more sources
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Physical Coupling of Kazarian Galaxies with Surrounding Galaxies
Astrophysics, 2003Results from a statistical study of Kazarian galaxies and the objects surrounding them are presented. It is shown that: (1) the sample of Kazarian galaxies up to 16m.0 is complete. (2) Roughly 35.7% of the Kazarian galaxies are members of clusters, 14.0% of groups, and 13.6% of binary systems, while 36.7% are single galaxies.
M. A. Kazarian, J. R. Martirosian
openaire +1 more source
2013
This chapter examines galaxies in some detail from a largely theoretical perspective. Along the way, one must bear in mind that, although the described progression of events in this chapter is plausible, at this time it is only a conjecture in the minds of theorists that has not yet been confirmed by observational data.
Abraham Loeb, Steven R. Furlanetto
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This chapter examines galaxies in some detail from a largely theoretical perspective. Along the way, one must bear in mind that, although the described progression of events in this chapter is plausible, at this time it is only a conjecture in the minds of theorists that has not yet been confirmed by observational data.
Abraham Loeb, Steven R. Furlanetto
openaire +1 more source
Modelling galaxy clustering: is new physics needed in galaxy formation models? [PDF]
The clustering amplitude of galaxies depends on their intrinsic luminosity. We compare the properties of publicly available galaxy formation models with clustering measurements from the two-degree field galaxy redshift survey. The model predictions show the same qualitative behaviour as the data but fail to match the observations at the level of ...
CARLOS Frenk +2 more
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The Physics of Stars and Galaxies
2020In this chapter we will be considering in detail the astrophysical building blocks of the Universe, stars. We first overview their main physical properties and life cycle, including their three possible end states: as white dwarfs, neutron stars, or black holes.
openaire +1 more source

