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The Cassiopeia A Supernova Was of Type IIb
Oliver Krause, Stephan M. Birkmann, Tomonori Usuda, Takashi Hattori, Miwa Goto, George H. Rieke and Karl A. Misselt
New Series, Vol. 320, No. 5880 (May 30, 2008), pp. 1195-1197
Published by: American Association for the Advancement of Science
Stable URL: http://www.jstor.org/stable/20054836
Page Count: 3
You can always find the topics here!Topics: Supernovae, Images, Brightness, Hydrogen, Stellar progenitors, Emission spectra, Visible spectrum, Helium, Wavelengths, Interstellar clouds
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Cassiopeia A is the youngest supernova remnant known in the Milky Way and a unique laboratory for supernova physics. We present an optical spectrum of the Cassiopeia A supernova near maximum brightness, obtained from observations of a scattered light echo more than three centuries after the direct light of the explosion swept past Earth. The spectrum shows that Cassipeia A was a type IIB supernova and originated from the collapse of the helium core of a red supergiant that had lost most of its hydrogen envelope before exploding. Our finding concludes a long-standing debate on the Cassiopeia A progenitor and provides new insight supernova physics by linking the properties of the explosion to the wealth of knowledge about its remnant.
Science © 2008 American Association for the Advancement of Science