Theoretical investigation of Sb-like sequence: Sb I, Te II, I III, Xe IV, and Cs V-Reference-Cited by-同舟云学术

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Theoretical investigation of Sb-like sequence: Sb I, Te II, I III, Xe IV, and Cs V

Published:2023-07 Issue: Volume:152 Page:101585
ISSN:0092-640X
Container-title:Atomic Data and Nuclear Data Tables
language:en
Short-container-title:Atomic Data and Nuclear Data Tables

Author:

Radžiūtė L.^ORCID,Gaigalas G.

Publisher

Elsevier BV

Subject

Nuclear and High Energy Physics,Atomic and Molecular Physics, and Optics

Reference66 articles.

1. The R-process Alliance: A Nearly Complete R-process Abundance Template Derived from Ultraviolet Spectroscopy of the R-process-enhanced Metal-poor Star HD 222925*

2. DETECTION OF THE SECOND r -PROCESS PEAK ELEMENT TELLURIUM IN METAL-POOR STARS,

3. Neutron-capture Elements in Planetary Nebulae: First Detections of Near-infrared [Te iii] and [Br v] Emission Lines

4. Tungsten versus Selenium as a potential source of kilonova nebular emission observed by Spitzer

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1. Theoretical Investigation of the Ge Isoelectronic Sequence;Journal of Physical and Chemical Reference Data;2024-08-13

2. Relativistic configuration interaction calculations on Kα X-ray satellites of Rb XXXVI to Rb XXVIII;The European Physical Journal Plus;2024-06-10

3. Theoretical study on Mα transition parameters of He-like to C-like cobalt ions;Journal of Physical and Chemical Reference Data;2024-04-04

4. Extended calculations of energy levels and transition rates for Yb LVII;Zeitschrift für Naturforschung A;2024-01-04

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