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Paczynski yıldız modellemesinde kullanılmak için opaklık tabloları ve onların yıldız evrimlerine etkileri

Year 2019, Volume: 21 Issue: 2, 578 - 589, 28.06.2019
https://doi.org/10.25092/baunfbed.624541

Abstract

Yıldız modellemede Paczyski ’nin ücretsiz programı GOB’a uygulanabilir bir formatta kullanmak için opaklık tabloları oluşturduk. Tablolarımız, Lagrange interpolasyon yöntemi kullanılarak düşük metal içerikli zarflar için Allard ve Weiss ’in tablolarından elde edilmiştir. Bu, verilen hidrojen (X ), helyum (Y) ve metallerin (Z) oranları ile yoğunluk ve sıcaklığın sayısal bir fonksiyonu olarak doğru opaklıkların elde edilmesini sağlar. Inlek ve grubu  opaklık etkilerini yüksek kalitede modern gözlemsel verilerden kontrol etmenin bağımsız olarak mümkün olduğunu göstermiştir. Bu tablolar bu tarz amaçlar için yararlı olacaktır.  

References

  • Schwarzschild, M., Structure and evolution of the stars, Princeton University Press, New Jersey, (1958).
  • Carson, T.R., Analytic formulae for Coulomb dipole transitions, Astronomy and Astrophysics Supplement Series,75, 385-389, (1988).
  • Iglesias, C. A., Rogers, F. J., Updated opal opacities, The Astrophysical Journal, 464, 943-953, ( 1996).
  • Peter L. Smith, Claas Heise, Jim R. Esmond, Robert L. Kurucz https://www.cfa.harvard.edu/amp/ampdata/kurucz23/sekur.html, (29.01.2019)
  • Rogers, F.J.& Iglesias, Iglesias, C. A., Radiative atomic Rosseland mean opacity tables, The Astrophysical Journal Supplement Series,79, 507-568, (1992).
  • Badnell, N.R., Bautista, M.A., Bulter, K., Delahaye, F., Mendoza, C., Palmeri, P., Zeippen, C.J., Seaton, M.J., Updated opacities from the opacity project, Monthly Notices of the Royal Astronomical Society, 360, 458-464, ( 2005).
  • Blancard, C., Cosse, P., Faussurier,G., Solar mixture opacity calculations using detailed configuration and level accounting treatments, The Astrophysical Journal, 745, 10, (2012).
  • Mondet,G., Blancard, C., Cosse, P., Faussurier,G., Opacity calculations for solar mixtures, The Astrophysical Journal Supplement Series, 220, 2, ( 2015).
  • Allard, F., https://opalopacity.llnl.gov/existing.html, (29.01.2019).
  • Weiss, A., https://opalopacity.llnl.gov/existing.html, (29.01.2019).
  • Inlek, G., Boke, A., Yılmaz, O., Budding, E., Effects of opacity on stellar radii and their relevance to observational data, Turkish Journal of Physics, 32, 65-77, ( 2008).
  • Paczynski,B., Acta Astronomica, 2, 20, (1970).
  • Young, P. A., Mamajek, E. E., Arnett, D., Liebert, J., Observational Tests and Predictive Stellar Evolution, The Astrophysical Journal, 556, 230-244, ( 2001).
  • Mathews, J.H., Numerical Methods For Mathematics Science and Engineering, A Simon and Schuster Co., New Jersey, (1992).
  • Huebner, W. F., Merts, A. L., Magee, N. H., and Argo, M. F., Los Alamos Scientific Report LA-6760., (1977).
  • Colgan, J., Kilcrease,D.P., Magee, N.H., et al., A New Generation of Los Alamos Opacity Tables, The Astrophysical Journal, 817, 116, ( 2016).

Opacity tables for using in Paczynski stellar modelling and their effects on stellar evolutions

Year 2019, Volume: 21 Issue: 2, 578 - 589, 28.06.2019
https://doi.org/10.25092/baunfbed.624541

Abstract

We have constructed opacity tables for using in stellar modelling in a format particularly applicable to the Paczynski  freeware program GOB.  Our tables are derived from those of Allard  and Weiss  for lower metal content envelopes, using the Lagrange interpolation method. This allows accurate opacities to be given as numerical functions of density and temperature with given proportions of hydrogen (X), helium (Y), and ‘metals’ (Z). Inlek et al.  showed that it is possible independently to check opacity effects from modern high-quality observational data. These tables will be useful for such purposes.

References

  • Schwarzschild, M., Structure and evolution of the stars, Princeton University Press, New Jersey, (1958).
  • Carson, T.R., Analytic formulae for Coulomb dipole transitions, Astronomy and Astrophysics Supplement Series,75, 385-389, (1988).
  • Iglesias, C. A., Rogers, F. J., Updated opal opacities, The Astrophysical Journal, 464, 943-953, ( 1996).
  • Peter L. Smith, Claas Heise, Jim R. Esmond, Robert L. Kurucz https://www.cfa.harvard.edu/amp/ampdata/kurucz23/sekur.html, (29.01.2019)
  • Rogers, F.J.& Iglesias, Iglesias, C. A., Radiative atomic Rosseland mean opacity tables, The Astrophysical Journal Supplement Series,79, 507-568, (1992).
  • Badnell, N.R., Bautista, M.A., Bulter, K., Delahaye, F., Mendoza, C., Palmeri, P., Zeippen, C.J., Seaton, M.J., Updated opacities from the opacity project, Monthly Notices of the Royal Astronomical Society, 360, 458-464, ( 2005).
  • Blancard, C., Cosse, P., Faussurier,G., Solar mixture opacity calculations using detailed configuration and level accounting treatments, The Astrophysical Journal, 745, 10, (2012).
  • Mondet,G., Blancard, C., Cosse, P., Faussurier,G., Opacity calculations for solar mixtures, The Astrophysical Journal Supplement Series, 220, 2, ( 2015).
  • Allard, F., https://opalopacity.llnl.gov/existing.html, (29.01.2019).
  • Weiss, A., https://opalopacity.llnl.gov/existing.html, (29.01.2019).
  • Inlek, G., Boke, A., Yılmaz, O., Budding, E., Effects of opacity on stellar radii and their relevance to observational data, Turkish Journal of Physics, 32, 65-77, ( 2008).
  • Paczynski,B., Acta Astronomica, 2, 20, (1970).
  • Young, P. A., Mamajek, E. E., Arnett, D., Liebert, J., Observational Tests and Predictive Stellar Evolution, The Astrophysical Journal, 556, 230-244, ( 2001).
  • Mathews, J.H., Numerical Methods For Mathematics Science and Engineering, A Simon and Schuster Co., New Jersey, (1992).
  • Huebner, W. F., Merts, A. L., Magee, N. H., and Argo, M. F., Los Alamos Scientific Report LA-6760., (1977).
  • Colgan, J., Kilcrease,D.P., Magee, N.H., et al., A New Generation of Los Alamos Opacity Tables, The Astrophysical Journal, 817, 116, ( 2016).
There are 16 citations in total.

Details

Primary Language English
Journal Section Research Articles
Authors

Gülay İnlek 0000-0002-4884-1437

Publication Date June 28, 2019
Submission Date December 27, 2018
Published in Issue Year 2019 Volume: 21 Issue: 2

Cite

APA İnlek, G. (2019). Opacity tables for using in Paczynski stellar modelling and their effects on stellar evolutions. Balıkesir Üniversitesi Fen Bilimleri Enstitüsü Dergisi, 21(2), 578-589. https://doi.org/10.25092/baunfbed.624541
AMA İnlek G. Opacity tables for using in Paczynski stellar modelling and their effects on stellar evolutions. BAUN Fen. Bil. Enst. Dergisi. June 2019;21(2):578-589. doi:10.25092/baunfbed.624541
Chicago İnlek, Gülay. “Opacity Tables for Using in Paczynski Stellar Modelling and Their Effects on Stellar Evolutions”. Balıkesir Üniversitesi Fen Bilimleri Enstitüsü Dergisi 21, no. 2 (June 2019): 578-89. https://doi.org/10.25092/baunfbed.624541.
EndNote İnlek G (June 1, 2019) Opacity tables for using in Paczynski stellar modelling and their effects on stellar evolutions. Balıkesir Üniversitesi Fen Bilimleri Enstitüsü Dergisi 21 2 578–589.
IEEE G. İnlek, “Opacity tables for using in Paczynski stellar modelling and their effects on stellar evolutions”, BAUN Fen. Bil. Enst. Dergisi, vol. 21, no. 2, pp. 578–589, 2019, doi: 10.25092/baunfbed.624541.
ISNAD İnlek, Gülay. “Opacity Tables for Using in Paczynski Stellar Modelling and Their Effects on Stellar Evolutions”. Balıkesir Üniversitesi Fen Bilimleri Enstitüsü Dergisi 21/2 (June 2019), 578-589. https://doi.org/10.25092/baunfbed.624541.
JAMA İnlek G. Opacity tables for using in Paczynski stellar modelling and their effects on stellar evolutions. BAUN Fen. Bil. Enst. Dergisi. 2019;21:578–589.
MLA İnlek, Gülay. “Opacity Tables for Using in Paczynski Stellar Modelling and Their Effects on Stellar Evolutions”. Balıkesir Üniversitesi Fen Bilimleri Enstitüsü Dergisi, vol. 21, no. 2, 2019, pp. 578-89, doi:10.25092/baunfbed.624541.
Vancouver İnlek G. Opacity tables for using in Paczynski stellar modelling and their effects on stellar evolutions. BAUN Fen. Bil. Enst. Dergisi. 2019;21(2):578-89.

Cited By

Yeni opaklıkların yıldız modellerine etkisi
Balıkesir Üniversitesi Fen Bilimleri Enstitüsü Dergisi
Gülay İNLEK
https://doi.org/10.25092/baunfbed.893455