Not exact matches
And Andromeda offers another advantage, according to Pawlowski: «Because you see the
galaxy almost
edge - on, you can look at the
line - of - sight velocities of its satellites to see the ones that are approaching and those that are receding, so it very clearly presents as a rotating disk.»
The skinny black
line on a plot of stellar rotation speed versus distance was expected to go down — stars close to the galactic center should orbit faster than stars at the
edge because all the mass concentrated at the center of the
galaxy pulls most powerfully on the closest stars.
This is a unique NASA / ESA Hubble Space Telescope view of the disk
galaxy NGC 5866 tilted nearly
edge - on to our
line - of - sight (Credit: NASA, ESA, and The Hubble Heritage Team (STScI / AURA)-RRB-
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