Hubble Characterizes the High-Velocity Smith Cloud

Hubble Characterizes the High-Velocity Smith Cloud

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News release ID: STScI-2016-04
Release Date: Jan 28, 2016
Image Use: Copyright
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The infalling Smith Cloud does not emit light at wavelengths that the Hubble Space Telescope is sensitive to. However, Hubble's Cosmic Origins Spectrograph can measure how the light from distant background objects is affected as it passes through the cloud. These measurements yield clues to the chemical composition of the cloud. By using these intergalactic forensics, Hubble astronomers trace the cloud's origin to the disk of our Milky Way. Combined ultraviolet and radio observations correlate to the cloud's infall velocities, providing solid evidence that the spectral features link to the cloud's dynamics.

Active Galaxies/Quasars, Cosmology, Galaxies, Infographics, Intergalactic Gas, Milky Way


Illustration: NASA, ESA, and A. Feild (STScI);
Science: NASA, ESA, and A. Fox (STScI)