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29:50 Modern Astronomy
Fall 1999
Lecture 26 ...October 27, 1999
Radio Galaxies and Quasars

tex2html_wrap_inline37 Watch the skies! Watch the skies! tex2html_wrap_inline32 On Sunday, Venus will be at its maximum angular distance from the Sun, tex2html_wrap_inline41 . Look at it and think about the geometry of the solar system.
tex2html_wrap_inline32 Over the next month, check out position of Moon relative to Jupiter and Saturn. It will clearly illustrate the tex2html_wrap_inline45 inclination of the Moon's orbit to the plane of the ecliptic.

tex2html_wrap_inline47 Contour map of 3C79, typical luminous radio galaxy. Radio galaxies have up to tex2html_wrap_inline49 times the radio power output of the Milky Way.
The distance to 3C79 is 1097 Megaparsecs! This is to be compared with the distance to the Andromeda galaxy of 0.63 Megaparsecs.

Think of distance modulus and how faint even the brightest stars must appear in 3C79. The whole galaxy is a fuzzy little smear on long exposure photos with big telescopes. Its apparent magnitude (the whole galaxy which is substantially more luminous than the Milky Way) is 18.6.

How do we know this? The answer is crucial to appreciating the nature of the Quasars. Return with us now to the thrilling days of yesteryear....
In the 1920's Edwin Hubble made two major discoveries: (1) the ``Nebulae'' were galaxies, (2) Galaxy spectra showed an odd feature.
tex2html_wrap_inline47 Diagram showing stylized spectrum of nearby galaxy, with rest wavelengths.

Question for audience: What does this mean?

Conclusion from Hubble's investigations: galaxies in all directions are moving away from us. Even more odd, the further away they are, the faster they are moving.

tex2html_wrap_inline47 Diagram showing Hubble's Law in graphical form.
This discovery is given in the form of an equation as

equation12

where tex2html_wrap_inline55 is the speed at which the galaxy is receding from us (kilometers/sec) d is the distance (in Megaparsecs), and tex2html_wrap_inline59 is the Hubble Constant in units of kilometers/sec/Megaparsec. Determination of the precise value of the Hubble constant has been and continues to be one of the primary goals of observational astronomy. The current best estimate is tex2html_wrap_inline61 kilometers/sec/Megaparsec.

The implications of Hubble's Law are philosophically staggering, but we will wait to discuss them when we talk about Cosmology. In the meanwhile we will use it as a distance determination method.

Let's work out an example. 3C79 has a measured recession speed of tex2html_wrap_inline63 km/sec. Therefore tex2html_wrap_inline65 .
tex2html_wrap_inline67 , so
tex2html_wrap_inline69 Megaparsecs.

This is the way we determine the distances to essentially all extragalactic objects more distance than the Virgo Cluster.

Quasars

Return with us now to those thrilling days of yesteryear... By around 1960 astronomers were realizing many of the brightest radio sources could not be definitely identified with elliptical galaxies.
tex2html_wrap_inline47 Picture of Virgo cluster
Examples were 3C48 and 3C273.

With improvements in radio astronomy, they were able to make precise measurements of the position on the sky of these two quasars, and saw that they coincided with starlike objects. Thus was born the class of astronomical objects called Quasi-Stellar Radio Sources.
tex2html_wrap_inline47 Look at Figure 24.2 from book showing spectrum of 3C273.

3C273 has a redshift of 0.16. Smaller than 3C79, but 3C273 is a 12th magnitude object ... you could image it for your lab project.

tex2html_wrap_inline32 If we use Hubble's Law to calculate its distance, then use its apparent magnitude to calculate its absolute magnitude, we end up with an incredibly brilliant object, brighter than any galaxy. And it doesn't look like a galaxy.

As time went on, thousands of these objects were discovered, and they represented one of the more enigmatic objects in astronomy. They were featured in an episode of Outer Limits in which scientists were driven nuts by ``Quasar Rays''.

For these Quasars, the redshifts ranged up to z=4.4 and beyond. For such larger redshifts you need to use a more general expression for the Doppler effect. Look at Figure 24.3 of your book for a more general distance-recession velocity relationship.

Think about the concept of ``Look-Back Time'' to these objects.

For about 30 years there was a huge controversy about the nature of Quasars. The orthodox viewpoint was that they were extragalactic objects, at the distances indicated by Hubble's Law, and that they were due to enormously brilliant phenomena in the centers of galaxies.

The heterodox viewpoint was that they were an entirely different class of astronomical object.

We now know that the orthodox viewpoint is correct. The real proof was given by Hubble Space Telescope images which showed the galaxy ``underneath'' the brilliant Quasars.
tex2html_wrap_inline47 Blackboard drawing of Quasar model.
tex2html_wrap_inline47 HST images of nearby Quasars

Other Topics
tex2html_wrap_inline32 Quasars as cosmic ghosts.
tex2html_wrap_inline32 The turn-on time for Quasars.
tex2html_wrap_inline32 What is going on in Quasars and Radio Galaxies.




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Steve Spangler
Wed Oct 27 11:08:03 CDT 1999