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Dataset on Stark broadening of Te II spectral lines.

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Title: Dataset on Stark broadening of Te II spectral lines.
Authors: Majlinger, Zlatko1 (AUTHOR), Dimitrijević, Milan S.1,2 (AUTHOR), Srećković, Vladimir A.1,3 (AUTHOR) vlada@ipb.ac.rs
Source: Advances in Space Research. Feb2026, Vol. 77 Issue 3, p4092-4097. 6p.
Subjects: Spectral lines, Tellurium, Ions, Stellar spectra, Collision broadening, Electron density, Temperature, Plasma diagnostics
Abstract: Stark widths for eight spectral lines of singly charged tellurium ion (Te II) have been calculated with the help of the modified semiempirical method. The calculations have been performed for a temperature range from 5 000 K up to 100 000 K and electron density of N e = 10 17 cm−3. Employing the obtained results, we investigated the influence of Stark broadening of Te II spectral lines to test the importance of the broadening by electron impacts in stellar spectra. Examples of the importance of Stark broadening in comparison with thermal Doppler broadening in atmospheres of spectral class DA, DB white dwarfs as well as A-type stars are presented. The newly acquired data will be important also for various modeling and laboratory plasma analysis. [ABSTRACT FROM AUTHOR]
Copyright of Advances in Space Research is the property of Pergamon Press - An Imprint of Elsevier Science and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
Database: Engineering Source
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Header DbId: egs
DbLabel: Engineering Source
An: 191270645
AccessLevel: 6
PubType: Academic Journal
PubTypeId: academicJournal
PreciseRelevancyScore: 0
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Items – Name: Title
  Label: Title
  Group: Ti
  Data: Dataset on Stark broadening of Te II spectral lines.
– Name: Author
  Label: Authors
  Group: Au
  Data: <searchLink fieldCode="AR" term="%22Majlinger%2C+Zlatko%22">Majlinger, Zlatko</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Dimitrijević%2C+Milan+S%2E%22">Dimitrijević, Milan S.</searchLink><relatesTo>1,2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Srećković%2C+Vladimir+A%2E%22">Srećković, Vladimir A.</searchLink><relatesTo>1,3</relatesTo> (AUTHOR)<i> vlada@ipb.ac.rs</i>
– Name: TitleSource
  Label: Source
  Group: Src
  Data: <searchLink fieldCode="JN" term="%22Advances+in+Space+Research%22">Advances in Space Research</searchLink>. Feb2026, Vol. 77 Issue 3, p4092-4097. 6p.
– Name: Subject
  Label: Subjects
  Group: Su
  Data: <searchLink fieldCode="DE" term="%22Spectral+lines%22">Spectral lines</searchLink><br /><searchLink fieldCode="DE" term="%22Tellurium%22">Tellurium</searchLink><br /><searchLink fieldCode="DE" term="%22Ions%22">Ions</searchLink><br /><searchLink fieldCode="DE" term="%22Stellar+spectra%22">Stellar spectra</searchLink><br /><searchLink fieldCode="DE" term="%22Collision+broadening%22">Collision broadening</searchLink><br /><searchLink fieldCode="DE" term="%22Electron+density%22">Electron density</searchLink><br /><searchLink fieldCode="DE" term="%22Temperature%22">Temperature</searchLink><br /><searchLink fieldCode="DE" term="%22Plasma+diagnostics%22">Plasma diagnostics</searchLink>
– Name: Abstract
  Label: Abstract
  Group: Ab
  Data: Stark widths for eight spectral lines of singly charged tellurium ion (Te II) have been calculated with the help of the modified semiempirical method. The calculations have been performed for a temperature range from 5 000 K up to 100 000 K and electron density of N e = 10 17 cm−3. Employing the obtained results, we investigated the influence of Stark broadening of Te II spectral lines to test the importance of the broadening by electron impacts in stellar spectra. Examples of the importance of Stark broadening in comparison with thermal Doppler broadening in atmospheres of spectral class DA, DB white dwarfs as well as A-type stars are presented. The newly acquired data will be important also for various modeling and laboratory plasma analysis. [ABSTRACT FROM AUTHOR]
– Name: AbstractSuppliedCopyright
  Label:
  Group: Ab
  Data: <i>Copyright of Advances in Space Research is the property of Pergamon Press - An Imprint of Elsevier Science and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
PLink https://search.ebscohost.com/login.aspx?direct=true&site=eds-live&db=egs&AN=191270645
RecordInfo BibRecord:
  BibEntity:
    Identifiers:
      – Type: doi
        Value: 10.1016/j.asr.2024.10.046
    Languages:
      – Code: eng
        Text: English
    PhysicalDescription:
      Pagination:
        PageCount: 6
        StartPage: 4092
    Subjects:
      – SubjectFull: Spectral lines
        Type: general
      – SubjectFull: Tellurium
        Type: general
      – SubjectFull: Ions
        Type: general
      – SubjectFull: Stellar spectra
        Type: general
      – SubjectFull: Collision broadening
        Type: general
      – SubjectFull: Electron density
        Type: general
      – SubjectFull: Temperature
        Type: general
      – SubjectFull: Plasma diagnostics
        Type: general
    Titles:
      – TitleFull: Dataset on Stark broadening of Te II spectral lines.
        Type: main
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      – PersonEntity:
          Name:
            NameFull: Majlinger, Zlatko
      – PersonEntity:
          Name:
            NameFull: Dimitrijević, Milan S.
      – PersonEntity:
          Name:
            NameFull: Srećković, Vladimir A.
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          Dates:
            – D: 01
              M: 02
              Text: Feb2026
              Type: published
              Y: 2026
          Identifiers:
            – Type: issn-print
              Value: 02731177
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            – Type: volume
              Value: 77
            – Type: issue
              Value: 3
          Titles:
            – TitleFull: Advances in Space Research
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