Description
Transcript: Most galaxies are made of stars, gas, and dust plus the ubiquitous dark matter. Elliptical and spiral galaxies contain different proportions of these materials, less dust and less gas for elliptical galaxies than spiral galaxies, but they are basically made of the same thing. The morphology of the galaxies is determined by their stellar orbits and the evolution of stellar populations. Their spectra are simply the sum of the spectra of billions of individual stars. However, certain galaxies have violent phenomena taking place in their centers. This can manifest in a number of ways, by a fierce starburst, by active x-ray emission, by non-thermal radio emission, or by gas moving with very high velocities near the nucleus. Collectively such galaxies are called active galaxies or AGN for active galactic nuclei.
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