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Dust Formation and Destruction in the Circumstellar Medium of Core-Collapse Supernovae

Dust Formation and Destruction in the Circumstellar Medium of Core-Collapse Supernovae Geoffrey C. Clayton Louisiana State University. Collaborators: Jen Andrews (LSU) Joe Gallagher (LSU) Mike Barlow (UCL)

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Dust Formation and Destruction in the Circumstellar Medium of Core-Collapse Supernovae

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  1. Dust Formation and Destruction in the Circumstellar Medium of Core-Collapse Supernovae Geoffrey C. Clayton Louisiana State University

  2. Collaborators: • Jen Andrews (LSU) • Joe Gallagher (LSU) • Mike Barlow (UCL) • Roger Wesson (UCL) • Jo Fabbri (UCL) • Margaret Meixner (STScI) • Massaki Otsuka (STScI) • Karl Gordon (STScI) • Barbara Ercolano (Exeter) • Ben Sugerman (Goucher) • Doug Welch (McMaster)

  3. QSO at z = 6.4 (Bertoldi et al. 2003).

  4. Dwek 1998

  5. Dwek 1998

  6. Dust Production SNe II (solid), Low mass stars (dotted), SNe Ia (dashed), destruction rate by astration (thick solid) (Dwek 1998)

  7. Barlow, Krause et al. 2010

  8. Barlow, Krause et al. 2010

  9. NGC 2397

  10. NGC 6946 SN 1917A, SN 1939C, SN 1948B, SN 1968D, SN 1969P, SN 1980K, SN 2002hh, SN 2004et, and SN 2008S SN 2002hh SN 2004et

  11. Signatures of dust formation in SNe • Asymmetric Emission Lines • IR emission • Fading in Visible • Increased extinction • Molecular formation

  12. SN 2003gd Mdust = 0.02 M☉

  13. SN 2002hh

  14. SN 2007od SN 2007it

  15. AG Car Hα Radio

  16. Mdust = 10-6 Mo SN 1987A 11.7 micron (red) + F625W (yellow) (Bouchet et al. 2006)

  17. CSM Interaction

  18. <-- M = 8 - 40 M☉ M = 1.4 - 25 M☉ -->

  19. Mass loss = 10 Mo Mgas/Mdust =100 Mgas = 9.9 M☉ Mdust = 0.1 M☉

  20. PISN SN with Mass = 140-260 Mo Schneider et al. 2004

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