Type Ia supernovae: Their origin and possible applications in cosmology

Science

Volumn 276, Issue 5317, 1997, Pages 1378-1382

  Nomoto, Ken'ichi ^a   Iwamoto, Koichi ^a   Kishimoto, Nobuhiro ^a  

^a UNIVERSITY OF TOKYO   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

ARGON; CALCIUM; CARBON; ELEMENT; HYDROGEN; IRON; ISOTOPE; MAGNESIUM; NEON; NICKEL; OXYGEN; SILICON; SULFUR;

ARTICLE; COSMOS; DENSITY; DEVICE; EVOLUTION; HYDRODYNAMICS; LIGHT; LUMINANCE; MODEL; PHOTOMETRY; PRIORITY JOURNAL; SPECTROSCOPY; SPECTRUM; VELOCITY;

ASTRONOMY; CARBON; ELEMENTS; EVOLUTION, PLANETARY; EXTRATERRESTRIAL ENVIRONMENT; LIGHT; NUCLEAR PHYSICS;

EID: 0030925554     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.276.5317.1378     Document Type: Article

References (67)

1. A. V. Filippenko, Annu. Rev. Astron. Astrophys., in press; D. Branch, K. Nomoto, A. V. Filippenko, Comments Astrophys. 15, 221 (1991).
2. A. V. Filippenko, Annu. Rev. Astron. Astrophys., in press; D. Branch, K. Nomoto, A. V. Filippenko, Comments Astrophys. 15, 221 (1991).
3. ⊙. For larger masses, pressures exerted by degenerate electrons cannot sustain the gravity because of the special relativistic effect.
4. Thermonuclear Supernovae, P. Ruiz-Lapuente, R. Canal, J. Isern, Eds. (Kluwer, Dordrecht, Netherlands, 1997); this book includes most of the recent progress in SNe la.
5. D. Branch and G. Tammann, Annu. Rev. Astron. Astrophys. 30, 359 (1992).
6. M. M. Phillips, Astrophys. J. 413, L105 (1993).
7. A. G. Riess, W. N. Press, R. P. Kirshner, ibid. 438, L17 (1995); ibid. 473, 88 (1996).
8. A. G. Riess, W. N. Press, R. P. Kirshner, ibid. 438, L17 (1995); ibid. 473, 88 (1996).
9. D. Branch, M. Livio, L. R. Yungelson, F. R. Boffi, E. Baron, Publ. Astron. Soc. Pac. 107, 717 (1995); A. Renzini, in IAU Colloquium 145, Supernovae and Supernova Remnants, R. McCray and Z. Wang, Eds. (Cambridge Univ. Press, Cambridge, 1996), pp. 77-85.
10. D. Branch, M. Livio, L. R. Yungelson, F. R. Boffi, E. Baron, Publ. Astron. Soc. Pac. 107, 717 (1995); A. Renzini, in IAU Colloquium 145, Supernovae and Supernova Remnants, R. McCray and Z. Wang, Eds. (Cambridge Univ. Press, Cambridge, 1996), pp. 77-85.
11. I. Iben Jr. and A. Tutukov, Astrophys. J. Suppl. Ser. 55, 335 (1984); R. Webbink, Astrophys. J. 277, 355 (1984).
12. I. Iben Jr. and A. Tutukov, Astrophys. J. Suppl. Ser. 55, 335 (1984); R. Webbink, Astrophys. J. 277, 355 (1984).
13. For example, K. Nomoto, Astrophys. J. 253, 798 (1982); _ and Y. Kondo, ibid. 367, L19 (1991); K. Nomoto et al., in Supernovae (Les Houches, Session LIV), S. Bludman et al., Eds. (Elsevier Science, Amsterdam, 1994), pp. 199-249.
14. For example, K. Nomoto, Astrophys. J. 253, 798 (1982); _ and Y. Kondo, ibid. 367, L19 (1991); K. Nomoto et al., in Supernovae (Les Houches, Session LIV), S. Bludman et al., Eds. (Elsevier Science, Amsterdam, 1994), pp. 199-249.
15. For example, K. Nomoto, Astrophys. J. 253, 798 (1982); _ and Y. Kondo, ibid. 367, L19 (1991); K. Nomoto et al., in Supernovae (Les Houches, Session LIV), S. Bludman et al., Eds. (Elsevier Science, Amsterdam, 1994), pp. 199-249.
16. I. Hachisu, M. Kato, K. Nomoto, Astrophys. J. 470, L97 (1996).
17. K. Nomoto, ibid. 257, 780 (1982); M. Hashimoto, K. Nomoto, K. Arai, K. Kaminisi, ibid. 307, 687 (1986).
18. K. Nomoto, ibid. 257, 780 (1982); M. Hashimoto, K. Nomoto, K. Arai, K. Kaminisi, ibid. 307, 687 (1986).
19. S. E. Woosley and T. A. Weaver, ibid. 423, 371 (1994).
20. E. P. J. van den Heuvel, D. Bhattacharya, K. Nomoto, S. A. Rappaport, Astron. Astrophys. 262, 97 (1992); S. A. Rappaport, R. DiStefano, J. Smith, Astrophys. J. 426, 692 (1994).
21. E. P. J. van den Heuvel, D. Bhattacharya, K. Nomoto, S. A. Rappaport, Astron. Astrophys. 262, 97 (1992); S. A. Rappaport, R. DiStefano, J. Smith, Astrophys. J. 426, 692 (1994).
22. P. Ruiz-Lapuente et al., Nature 365, 728 (1993).
23. W. D. Arnett, Nucleosynthesis and Supernovae (Princeton Univ. Press, Princeton, NJ, 1996); S. E. Woosley, in Supernovae, A. Petschek, Ed. (Springer, New York, 1990), pp. 182-212.
24. W. D. Arnett, Nucleosynthesis and Supernovae (Princeton Univ. Press, Princeton, NJ, 1996); S. E. Woosley, in Supernovae, A. Petschek, Ed. (Springer, New York, 1990), pp. 182-212.
25. Fe peak elements consist of mostly Fe and Ni with some Ti, V, Cr, Mn, and Co.
26. For example, J. Niemeyer and W. Hillebrandt, Astrophys. J. 452, 769 (1995); J. Niemeyer and S. E. Woosley, ibid. 475, 740 (1997).
27. For example, J. Niemeyer and W. Hillebrandt, Astrophys. J. 452, 769 (1995); J. Niemeyer and S. E. Woosley, ibid. 475, 740 (1997).
28. K. Nomoto, F.-K. Thielemann, K. Yokoi, ibid. 286, 644 (1984); F.-K. Thielemann, K. Nomoto, K. Yokoi, Astron. Astrophys. 158, 17 (1986); H. Yamaoka, T. Shigeyama, K. Nomoto, F.-K. Thielemann, Astrophys. J. 393, L55 (1992).
29. K. Nomoto, F.-K. Thielemann, K. Yokoi, ibid. 286, 644 (1984); F.-K. Thielemann, K. Nomoto, K. Yokoi, Astron. Astrophys. 158, 17 (1986); H. Yamaoka, T. Shigeyama, K. Nomoto, F.-K. Thielemann, Astrophys. J. 393, L55 (1992).
30. K. Nomoto, F.-K. Thielemann, K. Yokoi, ibid. 286, 644 (1984); F.-K. Thielemann, K. Nomoto, K. Yokoi, Astron. Astrophys. 158, 17 (1986); H. Yamaoka, T. Shigeyama, K. Nomoto, F.-K. Thielemann, Astrophys. J. 393, L55 (1992).
31. A. M. Khokhlov, Astron. Astrophys. 245, 114 (1991); S. E. Woosley and T. A. Weaver, in Supernovae (Les Houches, Session LIV), S. Bludman et al., Eds. (Elsevier Science, Amsterdam, 1994), pp. 63-154.
32. A. M. Khokhlov, Astron. Astrophys. 245, 114 (1991); S. E. Woosley and T. A. Weaver, in Supernovae (Les Houches, Session LIV), S. Bludman et al., Eds. (Elsevier Science, Amsterdam, 1994), pp. 63-154.
33. A. M. Khokhlov, Astron. Astrophys. 245, L25 (1991); W. D. Arnett and E. Livne, Astrophys. J. 427, 314 (1994).
34. A. M. Khokhlov, Astron. Astrophys. 245, L25 (1991); W. D. Arnett and E. Livne, Astrophys. J. 427, 314 (1994).
35. E. Livne, Astrophys. J. 354, L53 (1990).
36. T. Shigeyama, K. Nomoto, H. Yamaoka, F.-K. Thielemann, ibid. 386, L13 (1992); J. C. Wheeler and R. Harkness, Rep. Prog. Phys. 53, 1467 (1990).
37. T. Shigeyama, K. Nomoto, H. Yamaoka, F.-K. Thielemann, ibid. 386, L13 (1992); J. C. Wheeler and R. Harkness, Rep. Prog. Phys. 53, 1467 (1990).
38. P. Nugent, E. Baron, D. Branch, A. Fisher, P. Hauschildt, Astrophys. J., in press.
39. P. Höflich and A. Khokhlov, ibid. 457, 500 (1996).
40. For example, P. Mazzali, I. J. Danziger, M. Turatto, Astron. Astrophys. 297, 509 (1995); M. Turatto et al., Mon. Not. R. Astron. Soc. 283, 1 (1997).
41. For example, P. Mazzali, I. J. Danziger, M. Turatto, Astron. Astrophys. 297, 509 (1995); M. Turatto et al., Mon. Not. R. Astron. Soc. 283, 1 (1997).
42. P. Nugent, E. Baron, D. Branch, Astrophys. J. 455, L147 (1995).
43. For example, D. Jeffery et al., ibid. 397, 304 (1992); A. Fisher, D. Branch, P. Hoflich, A. Khokhlov, ibid. 447, L73 (1995); W. P. S. Meikle et al., Mon. Not. R. Astron. Soc. 281, 263 (1996).
44. For example, D. Jeffery et al., ibid. 397, 304 (1992); A. Fisher, D. Branch, P. Hoflich, A. Khokhlov, ibid. 447, L73 (1995); W. P. S. Meikle et al., Mon. Not. R. Astron. Soc. 281, 263 (1996).
45. For example, D. Jeffery et al., ibid. 397, 304 (1992); A. Fisher, D. Branch, P. Hoflich, A. Khokhlov, ibid. 447, L73 (1995); W. P. S. Meikle et al., Mon. Not. R. Astron. Soc. 281, 263 (1996).
46. P. Höflich et al., Astrophys. J. 472, L81 (1996).
47. M. Hashimoto, K. Nomoto, F.-K. Thielemann, Astron. Astrophys. 210, L5 (1989); F.-K. Thielemann, K. Nomoto, M. Hashimoto, Astrophys. J. 460, 408 (1996); T. Tsujimoto et al., Mon. Not. R. Astron. Soc. 277, 945 (1995); see also S. E. Woosley and T. A. Weaver, Astrophys. J. Suppl. Ser. 101, 181 (1995).
48. M. Hashimoto, K. Nomoto, F.-K. Thielemann, Astron. Astrophys. 210, L5 (1989); F.-K. Thielemann, K. Nomoto, M. Hashimoto, Astrophys. J. 460, 408 (1996); T. Tsujimoto et al., Mon. Not. R. Astron. Soc. 277, 945 (1995); see also S. E. Woosley and T. A. Weaver, Astrophys. J. Suppl. Ser. 101, 181 (1995).
49. M. Hashimoto, K. Nomoto, F.-K. Thielemann, Astron. Astrophys. 210, L5 (1989); F.-K. Thielemann, K. Nomoto, M. Hashimoto, Astrophys. J. 460, 408 (1996); T. Tsujimoto et al., Mon. Not. R. Astron. Soc. 277, 945 (1995); see also S. E. Woosley and T. A. Weaver, Astrophys. J. Suppl. Ser. 101, 181 (1995).
50. M. Hashimoto, K. Nomoto, F.-K. Thielemann, Astron. Astrophys. 210, L5 (1989); F.-K. Thielemann, K. Nomoto, M. Hashimoto, Astrophys. J. 460, 408 (1996); T. Tsujimoto et al., Mon. Not. R. Astron. Soc. 277, 945 (1995); see also S. E. Woosley and T. A. Weaver, Astrophys. J. Suppl. Ser. 101, 181 (1995).
51. K. Nomoto et al., in (3), pp. 349-378.
52. S. van den Bergh and G. A. Tammann, Annu. Rev. Astron. Astrophys. 29, 363 (1991).
53. For example, Y. Yoshii, T. Tsujimoto, K. Nomoto, Astrophys. J. 462, 266 (1996).
54. M. Hamuy et al., Astron. J. 109, 1 (1995); ibid. 112, 2398 (1996).
55. M. Hamuy et al., Astron. J. 109, 1 (1995); ibid. 112, 2398 (1996).
56. A. Sandage et al., Astrophys. J. 460, L15 (1996); A. Saha et al., ibid., in press.
57. A. Sandage et al., Astrophys. J. 460, L15 (1996); A. Saha et al., ibid., in press.
58. B. E. Schaefer, ibid. 460, L19 (1996).
59. W. D. Arnett, D. Branch, J. C. Wheeler, Nature 314, 337 (1985).
60. D. Branch, P. Nugent, A. Fisher, in (3), pp. 715-734.
61. P. Ruiz-Lapuente, Astrophys. J. 465, L83 (1996).
62. The Supernova Cosmology Project: S. Perlmutter et al., ibid., in press; IAU Circular 6596 (1997).
63. The Supernova Cosmology Project: S. Perlmutter et al., ibid., in press; IAU Circular 6596 (1997).
64. The High-Z Supernova Search Team: B. Schmidt et al., IAU Circular 6602 (1997).
65. P. Ruiz-Lapuente, A. Burkert, R. Canal, Astrophys. J. 447, L69 (1995); R. Canal, P. Ruiz-Lapuente, A. Burkert, ibid. 456, L101 (1996).
66. P. Ruiz-Lapuente, A. Burkert, R. Canal, Astrophys. J. 447, L69 (1995); R. Canal, P. Ruiz-Lapuente, A. Burkert, ibid. 456, L101 (1996).
67. Supported in part by a grant-in-aid for scientific research (05242102, 06233101, 4227) and COE research (07CE2002) of the Ministry of Education, Science, and Culture of Japan.