Skip to main content
SpringerLink
Log in

Does the energy of type IIP supernovae depend on the stellar mass?

  • Published:
Astronomy Letters Aims and scope Submit manuscript

Abstract

The oxygen density in the central zone of the ejecta of nine type IIP supernovae (SNe IIP) at the nebular phase has been determined from the [O I] 6300, 6364 Å doublet lines. In combination with the known estimates for two supernovae, the results of measurements show that the oxygen densities on day 300 are distributed in a narrow range, (2.3 ± 1) × 109 cm−3. This result does not depend on the distance, extinction, and model assumptions. Analysis of the density distribution found leads to the conclusion that the SN IIP explosion energy increases with stellar mass.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Log in via an institution

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Institutional subscriptions

Similar content being viewed by others

References

  1. L. H. Aller, Physics of Thermal Gaseous Nebulae (Reidel, Dordrech, 1984).

    Book  Google Scholar 

  2. G. S. Bisnovatyi-Kogan, Sov. Astron. 14, 652 (1971).

    ADS  MathSciNet  Google Scholar 

  3. N. Chugai, Astron. Tsirk. 1525, 15 (1988).

    ADS  Google Scholar 

  4. N. Chugai, Astron. Lett. 18, 239 (1992).

    Google Scholar 

  5. N. Chugai, Astrophys. J. 428, L17 (1994).

    Article  ADS  Google Scholar 

  6. N. N. Chugai, S. I. Blinnikov, R. Cumming, et al., Mon. Not. R. Astron. Soc. 352, 1213 (2004).

    Article  ADS  Google Scholar 

  7. N. N. Chugai, S.N. Fabrika, O. N. Sholukhova, et al., Astron. Lett. 31, 792 (2005).

    Article  ADS  Google Scholar 

  8. A. Clocchiatti, S. Benetti, J. C. Wheeler, et al., Astron. J. 111, 1286 (1996).

    Article  ADS  Google Scholar 

  9. S. A. Colgate and R. H. White, Astrophys. J. 143, 626 (1966).

    Article  ADS  Google Scholar 

  10. R. G. Eastman, S. E. Woosley, T. A. Weaver, and Ph. A. Pinto, Astrophys. J. 430, 300 (1994).

    Article  ADS  Google Scholar 

  11. C. L. Fryer, Astrophys. J. 522, 413 (1999).

    Article  ADS  Google Scholar 

  12. R. W. Hanuschik, ESO Workshop on SN 1987A and other Supernovae, Ed. by I. J. Danziger and K. Kjär (ESO, Garchiong, 1991), p. 237.

    Google Scholar 

  13. M. Hamuy, Astrophys. J. 582, 905 (2003).

    Article  ADS  Google Scholar 

  14. A. Heger, C. L. Fryer, S. E. Woosley, et al., Astrophys. J. 591, 288 (2003).

    Article  ADS  Google Scholar 

  15. A. Heger, N. Langer, and S. E. Woosley, Astrophys. J. 528, 368 (2000).

    Article  ADS  Google Scholar 

  16. V. S. Imshennik, Sov. Astron. Lett. 18, 194 (1992).

    ADS  Google Scholar 

  17. E. Kankare, M. Ergon, F. Bufano, et al., Mon. Not. R. Astron. Soc. 424, 855 (2012).

    Article  ADS  Google Scholar 

  18. C. Kozma and C. Fransson, Astrophys. J. 390, 602 (1992).

    Article  ADS  Google Scholar 

  19. C. Kozma and C. Fransson, Astrophys. J. 497, 431 (1998).

    Article  ADS  Google Scholar 

  20. O. Krause, S.M. Birkmann, T. Usuda, et al., Science 320, 1195 (2008).

    Article  ADS  Google Scholar 

  21. D. C. Leonard, A. V. Filippenko, E. L. Gates, et al., Publ. Astron. Soc. Pacif. 114, 35 (2002).

    Article  ADS  Google Scholar 

  22. W. Li, S. Van Dyk, A. V. Filippenko, et al., Astrophys. J. 641, 1060 (2006).

    Article  ADS  Google Scholar 

  23. W. Liu and A. Dalgarno, Astrophys. J. 454, 472 (1995).

    Article  ADS  Google Scholar 

  24. J. R. Maund, S. J. Smartt, and I. J. Danziger, Mon. Not. R. Astron. Soc. 364L, 33 (2005).

    ADS  Google Scholar 

  25. W. P. S. Meikle, R. Kotak, D. Farrah, et al., Astrophys. J. 732, 109 (2011).

    Article  ADS  Google Scholar 

  26. J. W. Menzies, in Proceedings of the ESO Workshop on SN 1987A and Other Supernovae, Ed. by I. J. Danziger and K. Kjär (ESO, Garchiong, 1991), p. 209.

  27. S. G. Moiseenko and G. S. Bisnovatyi-Kogan, IAUS 279, 357 (2012).

    ADS  Google Scholar 

  28. E. Müller, B. Fryxell, and D. Arnett, Astron. Astrophys. 251, 505 (1991).

    ADS  Google Scholar 

  29. D. K. Nadyozhin, Mon. Not. R. Astron. Soc. 346, 97 (2003).

    Article  ADS  Google Scholar 

  30. H. Nieuwenhuijzen and C. de Jager, Astron. Astrophys. 231, 134 (1990).

    ADS  Google Scholar 

  31. A. Pastorello, S. Valenti, L. Zampieri, et al., Mon. Not. R. Astron. Soc. 394, 2266 (2009).

    Article  ADS  Google Scholar 

  32. M. M. Phillips, M. Hamuy, S. R. Heathcote, et al., Astron. J. 99, 1133 (1990).

    Article  ADS  Google Scholar 

  33. D. K. Sahu, G. C. Anupama, S. Srividya, and S. Muneer, Mon. Not. R. Astron. Soc. 372, 1315 (2006).

    Article  ADS  Google Scholar 

  34. J. M. Shull and M. van Steenberg, Astrophys. J. Suppl. Ser. 49, 351 (1982).

    Article  ADS  Google Scholar 

  35. S. J. Smartt, J. J. Eldridge, R. M. Crockett, and J. R. Maund, Mon. Not. R. Astron. Soc. 395, 1409 (2009).

    Article  ADS  Google Scholar 

  36. J. Sollerman, R. Cumming, and P. Lundqvist, Astrophys. J. 493, 933 (1998).

    Article  ADS  Google Scholar 

  37. J. Spyromilio and Ph. Pinto, in Proceedings of the ESO Workshop on SN 1987A and Other Supernovae, Ed. by I. J. Danziger and K. Kjär (ESO, Garchiong, 1991), p. 423.

  38. N. B. Suntzeff and P. Bouchet, in Supernovae, Ed. by S. E. Woosley (Springer, New York, 1991), p. 3.

  39. K. Takáts, M. L. Pumo, N. Elias-Rosa, et al., arXiv: 1311.2525 (2013).

  40. L. Tomasella, E. Cappellaro, M. Fraser, et al., Mon. Not. R. Astron. Soc., No. 1, 1813 (2013).

    Google Scholar 

  41. M. Turatto, P. A. Mazzali, T. R. Young, et al., Astrophys. J. 498, 129 (1998).

    Article  ADS  Google Scholar 

  42. M. Ugliano, H.-Th. Janka, A. Marek, and A. Arcones, Astrophys. J. 757, 69 (2012).

    Article  ADS  Google Scholar 

  43. V. Utrobin and N. Chugai, Astron. Astrophys. 461, 233 (2013).

    Article  ADS  Google Scholar 

  44. V. Utrobin and N. Chugai, Astron. Astrophys. 506, 829 (2009).

    Article  ADS  Google Scholar 

  45. V. Utrobin, Astron. Astrophys. 461, 233 (2007).

    Article  ADS  Google Scholar 

  46. P. Whitelock, R. Catchpole, and M. Feast, in Supernovae, Ed. by S. E. Woosley (Springer, New York, 1991), p. 15.

  47. S. E. Woosley, A. Heger, and T. A. Weaver, Rev. Mod. Phys. 74, 1015 (2002).

    Article  ADS  Google Scholar 

Download references

Author information

Authors and Affiliations

  1. Institute of Astronomy, Russian Academy of Sciences, ul. Pyatnitskaya 48, Moscow, 119017, Russia

    N. N. Chugai & V. P. Utrobin

  2. Institute for Theoretical and Experimental Physics, ul. Bolshaya Cheremushkinskaya 25, Moscow, 117218, Russia

    N. N. Chugai & V. P. Utrobin

Authors
  1. N. N. Chugai
    View author publications

    You can also search for this author in PubMed Google Scholar

  2. V. P. Utrobin
    View author publications

    You can also search for this author in PubMed Google Scholar

Corresponding author

Correspondence to N. N. Chugai.

Additional information

Original Russian Text © N.N. Chugai, V.P. Utrobin, 2014, published in Pis’ma v Astronomicheskiĭ Zhurnal, 2014, Vol. 40, No. 5, pp. 330–340.

Rights and permissions

Reprints and permissions

About this article

Check for updates. Verify currency and authenticity via CrossMark

Cite this article

Chugai, N.N., Utrobin, V.P. Does the energy of type IIP supernovae depend on the stellar mass?. Astron. Lett. 40, 291–300 (2014). https://doi.org/10.1134/S1063773714050016

Download citation

  • Received:

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1134/S1063773714050016

Keywords

Search

Navigation