Advertisement

Expected Changes of SNe with Redshift due to Evolution of Their Progenitors

  • Inma Domínguez
  • Peter Höflich
  • Oscar Straniero
  • Marco Limongi
  • Alessandro Chieffi
Conference paper
Part of the Springer Proceedings in Physics book series (SPPHY, volume 99)

Summary

We have analyzed the influence of the stellar populations, from which SN progenitors come, on the observational outcome, including the metal free Pop. III. We use our models to study the evolution of the progenitor, the subsequent explosion and the light curves. For Type Ia, the variation of the main sequence mass of the progenitor of the exploding WD produces an offset in the maximum-decline relation of 0.2 mag. This effect is critical for the use of high redshift Type Ia SNe as cosmological standard candles. In contrast, the metallicity does not change the above relation (at maximum, ΔM V ≤0.06 mag). For Type II, we find a dependence of the light curve properties with both main sequence mass and metallicity of the progenitor, and we identify a rather homogeneous subclass, “Extreme II-P,” that may be used as a quasi-standard candle. Note that, although not as good as Type Ia for distance determinations, Type II are expected to have occurred since the first stars were formed.

Keywords

Dark Energy Light Curve Light Curf Massive Star Stellar Population 
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.

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  1. 1.
    A. Albrecht, J. Weller: Astron. Astrophys. Suppl. 197, 6106 (2000)Google Scholar
  2. 2.
    D. Branch, W. Romanishing, E. Baron: Astrophys. J. 465, 73 (1996)CrossRefADSGoogle Scholar
  3. 3.
    E. Cappellaro et al.: Astron. Astrophys. 322, 421 (1997)ADSGoogle Scholar
  4. 4.
    A. Chieffi, O. Straniero: Astrophys. J. Suppl. 71, 48 (1989)CrossRefADSGoogle Scholar
  5. 5.
    A. Chieffi, M. Limongi, O. Straniero: Astrophys. J. 502, 737 (1998)CrossRefADSGoogle Scholar
  6. 6.
    A. Chieffi, M. Limongi: Astrophys. J. 577, 281 (2002)CrossRefADSGoogle Scholar
  7. 7.
    A. Chieffi, I. Domínguez, P. Höflich, M. Limongi, O. Straniero: Mon. Not. R. Astron. Soc. 345, 111 (2003)CrossRefADSGoogle Scholar
  8. 8.
    I. Domínguez, P. Höflich: Astrophys. J. 528, 854 (2000)CrossRefADSGoogle Scholar
  9. 9.
    I. Domínguez, P. Höflich, O. Straniero: Astrophys. J. 557, 279 (2001)CrossRefADSGoogle Scholar
  10. 10.
    A.V. Filippenko: In: Cosmic Explosions. eds. S. Holt, W.W. Zhang (AIP: New York, 2000)Google Scholar
  11. 11.
    M. Hamuy et al.: Astron. J. 120, 1479 (2000)CrossRefADSGoogle Scholar
  12. 12.
    M. Hamuy, P.A. Pinto: Astrophys. J. Lett. 566, L63 (2002)CrossRefADSGoogle Scholar
  13. 13.
    M. Hamuy: Astrophys. J. 582, 905 (2003)CrossRefADSGoogle Scholar
  14. 14.
    P. Höflich: Astrophys. J. 443, 89 (1995)CrossRefADSGoogle Scholar
  15. 15.
    P. Höflich, A. Khokhlov, J.C. Wheeler: Astrophys. J. 444, 831 (1995)CrossRefADSGoogle Scholar
  16. 16.
    P. Höflich, A. Khokhlov: Astrophys. J. 457, 500 (1996)CrossRefADSGoogle Scholar
  17. 17.
    P. Höflich, J.C. Wheeler, F.K. Thielemann: Astrophys. J. 495, 617 (1998)CrossRefADSGoogle Scholar
  18. 18.
    P. Höflich, K. Nomoto, H. Umeda, J.C. Wheeler: Astrophys. J. 528, 590 (2000)CrossRefADSGoogle Scholar
  19. 19.
    P. Höflich, O. Straniero, M. Limongi, I. Domínguez, A. Chieffi: Rev. Mex. Astron. Astrofis. Conf. Series 10, 157 (2001)ADSGoogle Scholar
  20. 20.
    P. Hoyle, W.A. Fowler: Astrophys. J. 132, 565 (1960)CrossRefADSGoogle Scholar
  21. 21.
    I.J. Iben, A.V. Tutukov: Astrophys. J. Suppl. 54, 335 (1984)CrossRefADSGoogle Scholar
  22. 22.
    V.D. Ivanov, M. Hamuy, P.A. Pinto: Astrophys. J. 542, 588 (2000)CrossRefADSGoogle Scholar
  23. 23.
    A. Khokhlov: Astrophys. J. 457, 695 (1995)CrossRefADSGoogle Scholar
  24. 24.
    E.J. Lentz, E. Baron, D. Branch, P. Hauschildt, P.E. Nugent: Astrophys. J. 530, 966 (2000)CrossRefADSGoogle Scholar
  25. 25.
    M. Limongi A. Chieffi A., O. Straniero: Astrophys. J. Suppl. 129, 625L (2000)CrossRefADSGoogle Scholar
  26. 26.
    J. Maza S. van den Bergh: Astrophys. J. 204, 519 (1976)CrossRefADSGoogle Scholar
  27. 27.
    J. Miralda-Escudé, M.J. Rees: Astrophys. J. 478, 57 (1997)CrossRefADSGoogle Scholar
  28. 28.
    J.C. Niemeyer, W. Hillebrandt: Astrophys. J. 452, 779 (1995)CrossRefADSGoogle Scholar
  29. 29.
    P.E. Nugent, E. Baron, P. Hauschildt, D. Branch: Astrophys. J. 485, 812 (1997)CrossRefADSGoogle Scholar
  30. 30.
    F. Patat, R. Barbon, E. Cappellaro, M. Turatto: Astron. Astrophys. 282, 731 (1994)ADSGoogle Scholar
  31. 31.
    S. Perlmutter et al.: Astrophys. J. 517, 565 (1999)CrossRefADSGoogle Scholar
  32. 32.
    M.M. Phillips et al.: Pub. Astron. Soc. Pacific 90, 592 (1987)CrossRefADSGoogle Scholar
  33. 33.
    M.M. Phillips P. Lira, N.B. Suntzeff, R.A. Schommer, M. Hamuy, J. Maza: Astron. J. 118, 1766 (1999)CrossRefADSGoogle Scholar
  34. 34.
    A.G. Riess, W.H. Press, R.P. Kirshner: Astrophys. J. 473, 588 (1996)CrossRefADSGoogle Scholar
  35. 35.
    B.P. Schmidt et al.: Astrophys. J. 507, 46 (1998)CrossRefADSGoogle Scholar
  36. 36.
    O. Straniero, A. Chieffi, M. Limongi: Astrophys. J. 490, 425 (1997)CrossRefADSGoogle Scholar
  37. 37.
    G. Tammann: In: NATO-ASI on Supernovae: A Survey of Current Research. eds. M.J. Rees, R.J. Stoneham (Reidel: Dordrecht, 1982) p. 371Google Scholar
  38. 38.
    L. Wang, P. Höflich, J.C. Wheeler: Astrophys. J. Lett. 487, L29 (1997)CrossRefADSGoogle Scholar
  39. 39.
    R.F. Webbink: Astrophys. J. 277, 355 (1984)CrossRefADSGoogle Scholar
  40. 40.
    J. Whelan, I. Iben, Jr.: Astrophys. J. 186, 1007 (1973)CrossRefADSGoogle Scholar
  41. 41.
    J.C. Wheeler, P. Höflich, R. Harkness, J. Spyromilio: Astrophys. J. 496, 908 (1998)CrossRefADSGoogle Scholar
  42. 42.
    S.E. Woosley, T.A. Weaver: Ann. Rev. Astron. Astrophys. 24, 205 (1986)CrossRefADSGoogle Scholar
  43. 43.
    T.R. Young, D. Branch: Astrophys. J. Lett. 342, L79 (1989)CrossRefADSGoogle Scholar

Copyright information

© Springer-Verlag Berlin Heidelberg 2005

Authors and Affiliations

  • Inma Domínguez
    • 1
  • Peter Höflich
    • 2
  • Oscar Straniero
    • 3
  • Marco Limongi
    • 4
  • Alessandro Chieffi
    • 5
  1. 1.Universidad de GranadaGranadaSpain
  2. 2.Universidad de TexasAustinUSA
  3. 3.INAF-Osservatorio Astronomico di ColluraniaTeramoItaly
  4. 4.INAF-Osservatorio Astronomico di RomaMonteporzioItaly
  5. 5.Istituto di Astrofisica SpazialeCNRRomaItaly

Personalised recommendations