NTT, Spitzer, and Chandra spectroscopy of SDSSJ095209.56+214313.3: The most 
luminous coronal-line supernova ever observed, or a stellar tidal disruption 
event?

Komossa, S.; Zhou, H.; Rau, A.; Dopita, M.; Gal-Yam, A.; Greiner, J.; Zuther, J.; Salvato, M.; Xu, D.; Lu, H.; Saxton, R.; Ajello, M.

doi:10.1088/0004-637X/701/1/105

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NTT, Spitzer, and Chandra spectroscopy of SDSSJ095209.56+214313.3: The most luminous coronal-line supernova ever observed, or a stellar tidal disruption event?

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Komossa, S.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Zhou, H.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Greiner, J.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons22348

Lu, H.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Komossa, S., Zhou, H., Rau, A., Dopita, M., Gal-Yam, A., Greiner, J., et al. (2009). NTT, Spitzer, and Chandra spectroscopy of SDSSJ095209.56+214313.3: The most luminous coronal-line supernova ever observed, or a stellar tidal disruption event? The Astrophysical Journal, 701(1), 105-121. doi:10.1088/0004-637X/701/1/105.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0011-BFC8-5

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