Identification of absorption lines of rare-earth elements in the region of the spectrum λλ 610.25–610.57 nm roAp stars, HD 101065, HD 134214, HD 137949, and HD 24712

Author:

Mykhailytska N. G.

Publisher

Allerton Press

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference27 articles.

1. N. G. Mikhailitskaya, “Analysis of Lines in Atmosphere of RoAp Star HD 24712,” Kinem. Fiz. Neb. Tel 23, 148–157 (2007) [Kinem. Phys. Celest. Bodies 23, 101 (2007)].

2. S. A. Khan, “Calculating Synthetic Stellar Spectra with Regard to Magnetic Field Effect and Stratification of Chemical Elements,” Kinem. Fiz. Neb. Tel 19, 534–547 (2003).

3. A. V. Shavrina, N. S. Polosukhina, S. Khan, et al., “Lithium and the 6Li/7Li Isotope Ratio in the Atmospheres of Some SharpLined RoAp Stars,” Astron. Zh. 83(6), 1–12 (2006).

4. A. V. Shavrina, V. P. Khalak, N. G. Mikhailitskaya, and N. S. Polosukhina, “Taking Into Account the Magnetic Splitting of Lines in the Determination of of Lithium Abundance in the Atmosphere of the RoAp Star HD 101065,” Kinem. Fiz. Neb. Tel 20, 43–52 (2004).

5. E. Biemont, P. Palmeri, and P. Quinet, “A New Database of Astrophysical Interest,” Astrophys. Space Sci. 269–270, 635–637 (1999); D.R.A.M. Database on Rare Earth at Mons. Univ., http://www.umh.ac.be/astro/dream.shtml

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