IRON ABUNDANCES IN THE ATMOSPHERES OF HD10700 and HD146233

Автор(и)

  • O. N. Ivanyuk Main Astronomical Observatory of NASU, Україна
  • Ya. V. Pavlenko Main Astronomical Observatory of NASU, Україна
  • J. S. Jenkins University of Santyago, Чилі
  • H.R.A. Jones University of Hertfordshire, Велика Британія
  • Yu. Lyubchik Main Astronomical Observatory of NASU, Україна
  • B. Kaminsky Main Astronomical Observatory of NASU, Україна
  • M. Kuznetsov Main Astronomical Observatory of NASU, Україна

DOI:

https://doi.org/10.18524/1810-4215.2010.23.84651

Ключові слова:

solar-type stars, properties, abundances

Анотація

There are many different means to determine physical parameters of stars and their abundances by spectral analysis. In our work we draw our attention to the rotational and microturbulenc velocities as well as metallicities for the stars of known effective temperature and surface gravity. We carried fits of LTE synthetic spectra to the observed spectra of HD10700 and HD146233. These stars are knows aa solar-twins except slightly higher rotational velocities in both cases and higher magnetical activity i of HD10700. We adopted ABEL software (Pavlenko Ya.V.) to fit to HD10700, HD146233 spectra obtained on Camino Observatory, Chilie. Selected stars looks like. We compare our results with previous work of Valenti and Fischer (2005).

Посилання

Allende Prieto C.: 2004. Astronomische Nachrichten, 325, 604.

Jenkin sJ.S., Jones H.R.A., Pavlenko Y., Pinfield D.J., Barnes J.R., Lyubchik Y.: 2008, A&A, 485, 571.

Kupka F., Piskunov N., Ryabchikova T.A., Stempels H.C., Weiss W.W,.: 1999. Astron. Astrophys. Suppl., 138, 119.

Pavlenko Ya.V. : 1997, Astron. Astrophys. Sci., 253, p.43

Pavlenko Ya.V., Jones H.R.A., Longmore A.J.: 2003, MNRAS, 345, 311

Sneden C., Johnson H.R., Krupp B.M.: 1976, ApJ, 204, 218.

Valenti J.A., Fischer D.A.: 2005, The Astrophysical Journal, 159, 141

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Опубліковано

2010-11-28

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