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银河系Ⅰa型超新星所占星系恒星数目比例

The supernova Ia ratio in milky way galaxy
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摘要 利用银河系三成分(晕、厚盘和薄盘)星系化学演化模型,在比较了计算结果和可观测量的基础上,得出:Ⅰa型超新星数目约占恒星总数目的0.03。 Use the chemical evolution model of three-zone(the halo thick disk and thin disk),on the basis of compared the theoretical calculation and the observational constrains, it is shown that the number of type I a supernova is 3 percent of the whole milk-way galaxiy stellars.
出处 《沧州师范学院学报》 2007年第3期37-38,共2页 Journal of Cangzhou Normal University
关键词 元素丰度 星系演化模型 观测约束 Element abundance Galactic chemical evolution model observational constrains.
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参考文献10

  • 1Pardi,M.C,&Ferrini,F,Matteucci F.Evolution of spiral galaxies.IV:The thick disk in the solar region as an intermediate collapse phase[].The Astrophysical Journal.1995
  • 2Bahcall J.N.Self–consistent determination of the total amount of matter near the sun[].The Astrophysical Journal.1984
  • 3Rana N.C.Chemical evolution of the galaxy[].Annual Review of Astronomy and Astrophysics.1991
  • 4Greggio L,&Renzini A.Thebinary model for type supernovae-theoretical rates[].A&A.1983
  • 5Edvardsson B et al.The chemical evolution of the galactic disk I analysis and results[].A&A.1993
  • 6Rocha-Pinto,H.et al.Chemical enrichment and star formation in the milky way disk I sample description and chromospheric age-metallicity relation[].A&A.2000
  • 7Barbuy,B,&Erdelyi-MENDES,m.Oxygen in old and thick disk stars[].A&A.1989
  • 8Chen,Nissen,et al.Chemical compotion of 90 F and G disk white stars[].A&AS.2000
  • 9Portinari et al.Galactic chemical enrichment with new metallicity dependent stellar yields[].A&A.1998
  • 10Schmidt M,et al.The Rate of Star Formation[].The Astrophysical Journal.1959

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