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Chandra Spectra of RW Aur A
Chandra spectra from the 2013 and 2017 observations. The sharp peak on the right side of the 2017 spectrum is a signature of a large amount of iron.
(Credit: NASA/CXC/MIT/H.M.Günther)
Chandra spectra from the 2013 and 2017 observations. The sharp peak on the right side of the 2017 spectrum is a signature of a large amount of iron.
(Credit: NASA/CXC/MIT/H.M.Günther)
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Illustration
Artist's illustration depicting the destruction of a young planet.
(Credit: NASA/CXC/M.Weiss)
Artist's illustration depicting the destruction of a young planet.
(Credit: NASA/CXC/M.Weiss)
Return to RW Aur A (July 18, 2018)
Revised: November 29, 2022