The LMC Galaxy in Glowing Gas
Explanation:
What goes on inside of a galaxy?
To help find out, astronomers from the
Magellanic Cloud Emission Line Survey
team imaged our neighboring
LMC galaxy
in spectacular detail and highlighted very specific colors of
light emitted by glowing gas.
The
above mosaic of over 1,500 images of the
Large Magellanic Cloud (LMC) is the result -- clicking on the image will bring
up an
image with much greater detail.
The colors highlighted on the mosaic are light emitted by
hydrogen (red),
oxygen (green), and
sulfur (yellow), while light from individual stars has been subtracted.
The mosaic shows what a busy and violent place the inside of the LMC really is.
Visible in the
above image are many small
planetary nebulas
pushed out by low mass stars, large
emission nebula of
ambient interstellar gas
set aglow by massive stars, and huge gaseous
supernova remnants cast off by massive stars
exploding.
The extended connected filaments are mostly connected supernova remnants.
The
LMC,
a familiar
sight to an unaided eye in the
southern hemisphere,
spans about 15,000 light years and lies only about 180,000
light years distant.
Authors & editors:
Robert Nemiroff
(MTU) &
Jerry Bonnell
(USRA)
NASA Web Site Statements, Warnings,
and Disclaimers
NASA Official: Jay Norris.
Specific
rights apply.
A service of:
LHEA at
NASA /
GSFC
& Michigan Tech. U.
