Description
Transcript: In the first billion or so years after the big bang or before the first epoch of galaxy formation, the universe was in the period called the dark ages. No stars had yet formed. Ironically, the universe was smaller, denser, and hotter than it is now, and much of the gas and intergalactic space was very highly ionized at temperatures of tens of thousands of degrees. But the gas could not cool and could not gravitationally collapse to form objects, so the universe was dark. At some point within the first billion years the first stars formed. Astronomers refer to these as Population III stars. They must have contained the tiniest amount of heavy elements because that’s when many of the first heavy elements were produced. Then starting with the stars, objects like globular clusters and small galaxies formed, and over the subsequent billions of years, by a series of mergers in the hierarchical structure formation scenario, galaxies assembled to produce the large galaxies we see around us today.
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