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N. Ben Nessib

3 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • middle author1
  • last author1

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR3
ORCID 0000-0002-2402-7561

identity via Semantic Scholar / OpenAlex

most citedThe STARK-B database as a resource for \textquotedblleft STARK" widths and shifts data: State of advancement and program of development

19 citations · 37 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2013★ 19 cited

The STARK-B database as a resource for \textquotedblleft STARK" widths and shifts data: State of advancement and program of development

Sylvie Sahal-Bréchot, Milan S. Dimitrijević, Nicolas Moreau +1

\textquotedblleft Stark" broadening theories and calculations have been extensively developed for about 50 years and can now be applied to many needs, especially for accurate spect…

astro-ph.SR2013★ 4 cited

The OIV 1407.3Å/1401.1Å emission-line ratio in a plasma

Nabil Ben Nessib, Norah Alonizan, Rabia Qindeel +2

Line ratio of O IV 1407.3 Å/1401.1 Å\- is calculated using mostly our own atomic and collisional data. Energy levels and oscillator strengths needed for this calculation have been…

astro-ph.SR2013★ 14 cited

Stark widths of Ar III spectral lines in the atmospheres of subdwarf B stars

Rafik Hamdi, Nabil Ben Nessib, Sylvie Sahal-Bréchot +1

Using semiclassical perturbation approach in impact approximation, we have calculated Stark widths for 32 spectral lines of doubly charged argon (Ar III). Oscillator strengths are…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.