galactic halo

'There is much dark matter, here in the galactic halo.

The gas may be interconnected to form a sort of galactic halo.

They point out that the galactic halo is not symmetric between north and south.

The cluster was in the galactic halo and, of course, the trip was a long one.

The Foe were found to be in a cluster of such systems just outside the galactic halo."

This is most likely interstellar medium that has been heated by the passage of the cluster through the galactic halo.

Now live in great comfort, in a habitat external to galactic halo, where they simply watch place of Assassins.

He predicted the existence of a hot galactic halo surrounding the Milky Way galaxy.

The galactic halo also contains many globular clusters.

IC 4499 is a loose globular cluster in the medium-far galactic halo.

What types of galactic halos and outflowing winds do star-forming galaxies produce?

Under such models, the large majority of baryons entering a galactic halo do so along these cosmic filaments.

"A stable ball of stars perhaps a hundred thousand of them orbiting around the main disc, in the Galactic halo."

The dark matter is more like a wave than a particle, and the galactic halos are giant systems of condensed bose liquid.

These measurements suggest there was a hiatus of almost 5 billion years between the formation of the galactic halo and the thin disk.

SX Phoenicis variables are found primarily in globular clusters and galactic halos.

Their assignment was to monitor the most important object in either Heechee or human cosmology, the kugelblitz that hung outside the galactic halo.

In 1924, Oort discovered the galactic halo, a group of stars orbiting the Milky Way but outside the main disk.

Stars with a retrograde orbit are more likely to be found in the galactic halo than in the galactic disk.

The galactic halo is an extended, roughly spherical component of a galaxy, which extends beyond the main, visible component.

HVCs are typically the coldest and densest components of the Galactic halo.

Subsequent enrichment of galactic halos occurred due to stellar nucleosynthesis and supernova nucleosynthesis.

HVCs in the galactic halo are destroyed through what is called the Kelvin-Helmholtz instability.

However, some stars inhabit a spheroidal halo or galactic spheroid, a type of galactic halo.

Galaxy discs tend to have more gas and dust, and younger stars than galactic bulges, or galactic haloes.