Results 211 to 220 of about 1,645,813 (249)

A large, long-lived, slowly-expanding superbubble across the Perseus arm. [PDF]

open access: yesNat Commun
Chen B   +7 more
europepmc   +1 more source

The Physics of Galaxy Cluster Outskirts [PDF]

open access: yesSpace Science Reviews, 2019
56 pages. Review paper.
Dominique Eckert   +2 more
exaly   +5 more sources

The physics of dissipational galaxy formation

open access: yesAstrophysical Journal, 1977
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

The Physics of Galaxy Formation [PDF]

open access: yesSpringer Theses, 2014
Claudia Lagos
exaly   +2 more sources

Physical Coupling of Kazarian Galaxies with Surrounding Galaxies

Astrophysics, 2003
Results 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

Physics of Galaxy Evolution

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
openaire   +1 more source

Modelling galaxy clustering: is new physics needed in galaxy formation models? [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2009
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
exaly   +4 more sources

The Physics of Stars and Galaxies

2020
In 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

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