Hubble Probes the Invisible Halo of a Galaxy
Hubble Probes the Invisible Halo of a Galaxy
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News release ID: STScI-2011-37
Release Date: Nov 17, 2011
Image Use: Copyright
About this image

Distant quasars serve as distant lighthouse beacons that shine through the gas-rich "fog" of hot plasma encircling galaxies. At ultraviolet wavelengths, Hubble's Cosmic Origins Spectrograph (COS) is sensitive to absorption from many ionized heavy elements, such as nitrogen, oxygen, and neon. COS's high sensitivity allows many galaxies that happen to lie in front of the much more distant quasars to be studied. The ionized heavy elements serve as proxies for estimating how much mass is in a galaxy's halo.


Tags
Active Galaxies/Quasars, Galaxies, Hubble Telescope, Illustrations

Credits

Illustration Credit: NASA, ESA, and A. Feild (STScI)

Science Credit: NASA, ESA, N. Lehner (University of Notre Dame), T. Tripp (University of Massachusetts, Amherst), and J. Tumlinson (STScI)