Description
Transcript: We’ve discovered a supermassive black hole in the center of our galaxy the Milky Way. However, it would violate the Copernican principle if the Milky Way were unique in any way, so astronomers anticipated black holes in other galaxies or other evidence of nuclear activity. There are two main things that astronomers search for when they are trying to detect a supermassive black hole in another galaxy. The first is a sharp peak or cusp in the light distribution, and the second is a high stellar velocity dispersion. The cusp in the light distribution is measured by imaging, the higher resolution the better, so usually this work is done from space with the Hubble Space Telescope. The spectroscopy is also best done from space where the smallest slit must be placed over the center of the galaxy to isolate the stellar motions in the very central regions. If a galaxy has a cusp in its light distribution and a high degree of stellar motion near the center then the implied mass to light ratio will be higher than any plausible stellar population, so dark, concentrated mass is indicated: a supermassive black hole.
Transcript: The fact that quasars are at large distances and have huge luminosities depends on the cosmological interpretation of their redshift. There are some crucial distinctions between galaxies and quasars as far as redshift goes. For galaxies they follow a Hubble relation where distance...
Published 07/28/11
Transcript: Quasars were mysterious when they were first discovered in the 1960s. But careful work showed that the quasar is surrounded by nebulosity, and eventually spectroscopy of the nebulosity showed that it was the light of stars in a normal galaxy. Thus quasar stands for quasi-stellar...
Published 07/28/11
Transcript: Astronomers at Caltech became interested in the newly accurate radio positions of strong sources in the sky. They focused in particular on two sources, 3C48 and 3C273 which appeared to be associated with bluish stars. Since normal stars like the Sun do not emit strong radio waves...
Published 07/28/11