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The journal article ``Discovery of a bright quasar without a massive host
galaxy'' in Nature 437, 381-384 (15 September 2005) describes
observations of the object HE0450-2958 made with the Hubble Space Telescope
(HST) and the Very Large Telescope (VLT). The article is available on-line through the
University subscription to Nature following the link on the class web site at
http://www.physics.louisville.edu/astro/students/590. A pdf version for
your use is on our computer system in the directory
/home/data/bright_quasar along with image files you will need.
After you have read the article and we have discussed it in class, answer the
questions that follow. A few points to keep in mind:
- The increase in the wavelength of spectral lines from distant galaxies
(and quasars) due to the expansion of the universe is given by the Hubble Law
where
is the velocity of recession and
is the distance of
the galaxy.
is the Hubble Constant, taken in this article to be 65
km/s-Mpc. Distance is measured in parsecs, the distance at which the parallax
of an object would be 1 second of arc. A parsec is also the distance at which 1
astronomical unit, the mean distance of the Earth from the Sun, would subtend an
angle of 1 second of arc. The velocity of recession is measured in km/s. An
Mpc is a ``megaparsec'',
parsecs.
- The velocity of recession implies a shift of wavelengths to the red due to
the Doppler effect. This change in wavelength is given exactly by
In the limit that
is small, this becomes
where
is positive when the galaxy is moving away from us.
- Absolute magnitude
is the magnitude an object would have if it were
10 parsecs away. It is related to the apparent magnitude
by
which follows from the definition of the magnitude scale and the inverse square
law for light flux.
Next: Questions
Up: A Bright Quasar
Previous: A Bright Quasar
John Kielkopf
2005-09-23