Aims. The main goal of this paper is to present accurate and extensive transition data for the P II ion. These data are useful in various astrophysical applications. Methods. The multiconfiguration Dirac-Hartree-Fock (MCDHF) and relativistic configuration interaction (RCI) methods, which are implemented in the general-purpose relativistic atomic structure package GRASP2K, were used in the present work. In the RCI calculations the transverse-photon (Breit) interaction, the vacuum polarization, and the self-energy corrections were included. Results. Energy spectra are presented for 48 even states of the 3S(2)3p(2) ,3s(2)3p{4p, 4f, 5p, 5f, 6p}, 3s3 p(2)3d configurations, and for 58 odd states of the 3s3p(3) , 3s(2)3p{3d, 4s, 4d, 5s, 5d, 6s} co...
Aims. We seek to present accurate and extensive transition data for the Zr III ion. These data are u...
Aims. Accurate atomic data for Ti II are essential for abundance analyses in astronomical objects. T...
Aims. Accurate atomic data for Ti II are essential for abundance analyses in astronomical objects. T...
Aims. The main goal of this paper is to present accurate and extensive transition data for the P II ...
Aims. The main goal of this paper is to present accurate and extensive transition data for the P II ...
Aims. The main goal of this paper is to present accurate and extensive transition data for the P II ...
Aims. The main goal of this paper is to present accurate and extensive transition data for the P II ...
Aims. The aim of this work is to present accurate and extensive results of energy spectra and transi...
Aims. The aim of this work is to present accurate and extensive results of energy spectra and transi...
Aims. The aim of this work is to present accurate and extensive results of energy spectra and transi...
Aims. The aim of this work is to present accurate and extensive results of energy spectra and transi...
Aims. The aim of this work is to present accurate and extensive results of energy spectra and transi...
Aims. The aim of this work is to present accurate and extensive results of energy spectra and transi...
Aims. We seek to present accurate and extensive transition data for the Zr III ion. These data are u...
Aims. We seek to present accurate and extensive transition data for the Zr III ion. These data are u...
Aims. We seek to present accurate and extensive transition data for the Zr III ion. These data are u...
Aims. Accurate atomic data for Ti II are essential for abundance analyses in astronomical objects. T...
Aims. Accurate atomic data for Ti II are essential for abundance analyses in astronomical objects. T...
Aims. The main goal of this paper is to present accurate and extensive transition data for the P II ...
Aims. The main goal of this paper is to present accurate and extensive transition data for the P II ...
Aims. The main goal of this paper is to present accurate and extensive transition data for the P II ...
Aims. The main goal of this paper is to present accurate and extensive transition data for the P II ...
Aims. The aim of this work is to present accurate and extensive results of energy spectra and transi...
Aims. The aim of this work is to present accurate and extensive results of energy spectra and transi...
Aims. The aim of this work is to present accurate and extensive results of energy spectra and transi...
Aims. The aim of this work is to present accurate and extensive results of energy spectra and transi...
Aims. The aim of this work is to present accurate and extensive results of energy spectra and transi...
Aims. The aim of this work is to present accurate and extensive results of energy spectra and transi...
Aims. We seek to present accurate and extensive transition data for the Zr III ion. These data are u...
Aims. We seek to present accurate and extensive transition data for the Zr III ion. These data are u...
Aims. We seek to present accurate and extensive transition data for the Zr III ion. These data are u...
Aims. Accurate atomic data for Ti II are essential for abundance analyses in astronomical objects. T...
Aims. Accurate atomic data for Ti II are essential for abundance analyses in astronomical objects. T...