Quasars

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In the 1960s it was observed that certain objects emitting radio waves but thought to be stars had very unusual optical spectra. It was finally realized that the reason the spectra were so unusual is that the lines were Doppler shifted by a very large amount, corresponding to velocities away from us that were significant fractions of the speed of light. The reason that it took some time to come to this conclusion is that, because these objects were thought to be relatively nearby stars, no one had any reason to believe they should be receding from us at such velocities.

Quasars and QSOs

These objects were named Quasistellar Radio Sources (meaning "star-like radio sources") which was soon contracted to quasars. Later, it was found that many similar objects did not emit radio waves. These were termed Quasistellar Objects or QSOs. Now, all of these are often termed quasars (Only about 1% of the quasars discovered to date have detectable radio emission).

Here are some Hubble Space Telescope quasar images, and the following figure shows the quasar 3C273, which was the first quasar discovered and is also the quasar with the greatest apparent brightness. It will be discussed further below.

The quasar 3C273. Left image shows the quasar and the jet. Right image superposes on this contours of radio frequency intensity. The sharp radial lines from the quasar are optical spike artifacts because of its brightness