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Optical and Near-IR Observations of SN 1998bw

  • Ferdinando Patat
Conference paper
Part of the Springer Proceedings in Physics book series (SPPHY, volume 99)

Summary

SN 1998bw, especially after the discovery of GRB 030329/SN 2003dh, seems to be the equivalent of the Rosetta stone for the SN/GRB connection. In this paper I review optical and near IR observations that have been carried out for this uncanny object, which has probably confirmed suspicions and ideas originally formulated in the early seventies of last century.

Keywords

Light Curve Blast Wave Expansion Velocity Maximum Light Wide Field Camera 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. 1.
    J.S. Bloom et al.: Nature 401, 453 (1999)CrossRefADSGoogle Scholar
  2. 2.
    D.D. Clayton, S.A. Colgate, G.J. Fishman: Astrophys. J. 155, 75 (1969)CrossRefADSGoogle Scholar
  3. 3.
    S.A. Colgate: Astrophys. J. 187, 333 (1974)CrossRefADSGoogle Scholar
  4. 4.
    A.V. Filippenko: IAUC 6969 (1998)Google Scholar
  5. 5.
    J.U. Fynbo et al.: Astrophys. J. Lett. 542, L89 (2000)CrossRefADSGoogle Scholar
  6. 6.
    T.J. Galama, P.M. Vreeswijk, E. Pian, F. Frontera, V. Doublier, J.F. Gonzalez: IAUC 6895 (1998)Google Scholar
  7. 7.
    T.J. Galama et al.: Nature 1395, 670 (1998)CrossRefADSGoogle Scholar
  8. 8.
    T.J. Galama et al.: Astron. Astrophys. Suppl. 138, 465 (1999)CrossRefADSGoogle Scholar
  9. 9.
    P. Garnavich, T. Matheson, E. W. Olszewski, P. Harding, K. Z. Stanek: IAUC 8108 (2003)Google Scholar
  10. 10.
    P. Höflich, J.C. Wheeler, L. Wang: Astrophys. J. 521, 179 (1999)CrossRefADSGoogle Scholar
  11. 11.
    K. Iwamoto et al.: Nature 395, 672 (1998)CrossRefADSGoogle Scholar
  12. 12.
    L.E. Kay, J.P. Halpern, K.M. Leighly, S. Heathcote, A.M. Magalhaes: IAUC 6969 (1998)Google Scholar
  13. 13.
    S.R. Kulkarni et al.: Nature 395, 663 (1998)CrossRefADSGoogle Scholar
  14. 14.
    C. Lidman, V. Doublier, J.F. Gonzalez, T. Augusteijn, O. Hainaut, H. Boehnhardt, F. Patat, B. Leibundgut: IAUC 6895 (1998)Google Scholar
  15. 15.
    P.A. Mazzali, K. Iwamoto, K. Nomoto: Astrophys. J. 545, 407 (2000)CrossRefADSGoogle Scholar
  16. 16.
    E.H. McKenzie, B.E. Schaefer: Pub. Astron. Soc. Pacific 111, 964 (1999)CrossRefADSGoogle Scholar
  17. 17.
    F. Patat, A. Piemonte: IAUC 6918 (1998)Google Scholar
  18. 18.
    F. Patat et al.: Astrophys. J. 555, 900 (2001)CrossRefADSGoogle Scholar
  19. 19.
    E. Pian et al.: Astron. Astrophys. Suppl. 138, 463 (1999)CrossRefADSGoogle Scholar
  20. 20.
    P. Soffita et al.: IAUC 6884 (1998)Google Scholar
  21. 21.
    J. Sollerman, C. Kozma, C., C. Fransson, B. Leibundgut, P. Lundqvist, F. Ryde, P. Woudt: Astrophys. J. Lett. 537, L127 (2000)CrossRefADSGoogle Scholar
  22. 22.
    J. Sollerman et al.: Astron. Astrophys. 386, 944 (2002)CrossRefADSGoogle Scholar
  23. 23.
    R.A. Stathakis et al.: Mon. Not. R. Astron. Soc. 314, 807 (2000)CrossRefADSGoogle Scholar

Copyright information

© Springer-Verlag Berlin Heidelberg 2005

Authors and Affiliations

  • Ferdinando Patat
    • 1
  1. 1.European Southern ObservatoryGarchingGermany

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