The inescapable conclusion, assuming that Newton's law of gravity (and the local physics description) holds on cosmological scales, that the visible galaxy was embedded in a much larger dark matter (DM) halo, which contributes roughly 50%–90% of the total mass of a galaxy. Search.
Learn vocabulary, terms, and more with flashcards, games, and other study tools. Start studying Quiz 12 Chapter 16.
The radial velocities are derived from the doppler shifted H-alpha lines (rest wavelength 6563 Angstroms). Learn vocabulary, terms, and more with flashcards, games, and other study tools. It has a lot of nonluminous (dark) matter in its outer regions. It has a lot of nonluminous (dark) matter in its outer regions Which feature of a galaxy seems to be related to the mass of the galaxy's central supermassive black hole? What does the flatness of the rotation curve shown here reveal about this galaxy? Search. Click here to see an example of how the rotation curve appears in the spectral image. These models were unable to predict the flatness of the observed rotation curve beyond the stellar disk. ... What type of galaxy is the most likely result of the process of the previous question> (A) ... What does the flatness of the rotation curve shown here reveal about this galaxy? What does the flatness of the rotation curve shown here reveal about this galaxy? Start studying kill me. The part of the galaxy including all matter in a spherical distribution around the center ... What does the flatness of the rotation curve shown here reveal about this galaxy? This is an image of the starburst galaxy NGC 1569. Then, the innermost regions are adjusted so that the disk is able to produce the observed rotation curve without a halo. Here, the mass to light, M/L, ratio is fixed for the different visible components, with values higher than about 10 being difficult to assign to a stellar population. Shown is the variation in the observed rotation velocity along the major axis. It has a lot of nonluminous (dark) matter in its outer regions. What does the flatness of the rotation curve shown here reveal about this galaxy?
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