Using the 6.5-meter Magellan telescope at Las Campanas, we have mapped
the galaxy M83 at unprecedented resolution. The seeing on the mountain
was 0.4 arcseconds for most of the observing run, and with the light gathering
power of the 6.5-meter telescope we were able to gather images comparable
to those made with the Hubble Space Telescope. What Hubble gains in resolution,
we gain in light gathering power. The result is a view of the galaxy M83
better than ever seen before. Dr. Barry Madore, Dr. Wendy Freedman, Ryan
Quadri (Harvey Mudd) and Dr. Bryan Penprase have taken these images, and
will study the images to look for evidence of asymptotic giant stars and
Cepheids. The result will be an improved understanding of
the distance to the galaxy, and of the evolution of the halo population of stars within the galaxy.
In the following section are links to large images of the galaxy M83. You can click on each image below to get a full size image on a separate browser.
Also you can see our gallery of images taken at the 6.5-meter telescope. It includes images of other galaxies such as IC4662, M83, NGC 2915, and NGC 5253.
Gallery of galaxy images taken during the March 2001 Las Campanas Observing run with Barry Madore, Wendy Freedman, Ryan Quadri, and Bryan Penprase
To get a view of what the galaxy M83 looks like, below is a link to a full color image of the galaxy taken by Dr. Barry Madore at the 100" DuPont telescope. This is the view of the galaxy which an inhabitant of an orbiting globular cluster might see. You can click on this image to get a larger view.
One of our main projects was to get information on the population of
stars at the edge of the galaxy. We used the 6.5-meter telescope to gather
images at progressively greater distances from the core of the galaxy.
In the images below you can see a montage of several images which march
out to greater distances from the center of the galaxy. At the edge is
the image of the faint stars in the halo of the galaxy. The outer image
was constructed using dozens of exposures with the 6.5-meter telescope
to reveal stars and galaxies that nobody has ever seen before! All the
images were made using the V and I filters -- we have mapped the V filter
to the blue channel and the I filter to the R and G channels to simulate
real color. The image below is reduced in size by half so you can see it
in your browser. The amount of information in the image is staggering --
as is the dynamic range of the image which falls from very bright to nearly
26th magnitude. The sharp changes in colors of the stars within the galaxy
is apparent, as the various stellar populations give light in blue or red
light depending on their age and luminosity.
The bright blue dots in the picture correspond to individual O and B stars in this galaxy.