Consider a star in the midplane of the Galactic disk with Galactic longitude l at a distance d from the Sun.
12.
By this measure, some of the stars across the galactic disk of Bmk 16 : 57, 21 August 2006 ( UTC)
13.
Though most galactic disks are flat because of their rate of rotation, their conformation can be changed, as is the case with this galaxy.
14.
Large enough superbubbles can blow through the entire galactic disk, releasing their energy into the surrounding galactic halo or even into the intergalactic medium.
15.
The results showed that typical halos extended to at least 1.3 million light-years into space from the luminous galactic disks, more than double the previous limit.
16.
The cluster appears to be producing a thermal chimney of ionized gas, caused by the interaction of the gas from the galactic disk with the galactic halo.
17.
The isotopic ratio of [ 12 C ] / [ 13 C ] was determined to be about or less than 50 % in the galactic disk.
18.
In the same way, the next rise in the galactic structure is blocking view of what lies beyond, which apparently is a significant portion of the galactic disk.
19.
Consequently, when discussing HVCs in the context of galactic evolution, the conversation is largely concerned with star formation and how the future star material fuels the galactic disk.
20.
The results showed that typical halos extended to at least 1 . 3 million light-years into space from the luminous galactic disks, more than double the previous limit.
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