Spectral analysis and calculations of line parameters for Xe-like Ce V-Reference-Cited by-同舟云学术

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Spectral analysis and calculations of line parameters for Xe-like Ce V

Published:2021-01 Issue: Volume:258 Page:107387
ISSN:0022-4073
Container-title:Journal of Quantitative Spectroscopy and Radiative Transfer
language:en
Short-container-title:Journal of Quantitative Spectroscopy and Radiative Transfer

Author:

Wajid Abdul,Tauheed A.,Jabeen S.

Funder

University Grants Commission

Aligarh Muslim University

Publisher

Elsevier BV

Subject

Spectroscopy,Atomic and Molecular Physics, and Optics,Radiation

Reference26 articles.

1. Stellar laboratories III. New Ba V, Ba VI, and Ba VII oscillator strengths and the barium abundance in the hot white dwarfs G191−B2B and RE 0503–289;Rauch;A&A,2014

2. Rare-earth elements in the atmosphere of the magnetic chemically peculiar star HD 144897. New classification of the Nd III spectrum;Ryabchikova;A & A,2006

3. First detection of bromine and antimony in hot stars;Werner;A & A,2018

4. Application of Laboratory Atomic Physics to Some Significant Stellar Chemical Composition Questions;Sneden;Atoms,2018

5. r-process lanthanide production and heating rates in kilonovae;Lippuner;Astrophys. J.,2015

Cited by 1 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Large-scale atomic data calculations in Ce V – X ions for application to early kilonova emission from neutron star mergers;Monthly Notices of the Royal Astronomical Society;2021-11-26

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