CHEMICAL COMPOSITIONS OF CRAB NEBULA FILAMENTS

Автор(и)

  • V. V. Holovatyy Department of Astrophysics of Ivan Franko National University, Україна
  • B. Ya. Melekh Department of Astrophysics of Ivan Franko National University, Україна
  • N. V. Havrylova Department of Astrophysics of Ivan Franko National University, Україна

DOI:

https://doi.org/10.18524/1810-4215.2013.26.81838

Ключові слова:

Crab Nebula, nebular diagnostics, photoionization modeling

Анотація

The chemical compositions in filaments of Crab Nebula are obtained using two methods: new Ionization Correction Factors taking in to account density in homogeneities f the nebular gas, and new 3-stages method based on the optimized photoionization modeling of the nebular gas.

Посилання

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Holovatyy V.V. et al.:1999, Izvest. Krymsk. astrophys. bserv., 96, 1.

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Melekh B.Ya.:2009, JPhS 13, 3, 3901.

Melekh B.Ya. et al.:2012, Odessa Astr. Publ., 25/2, 178.

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Опубліковано

2013-11-02

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