On the Stark broadening of the Re II spectral lines
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2023
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Prikaz svih podataka o dokumentuApstrakt
Stark broadening parameters - full widths at half maximum (FWHM) and shifts for 11 Re II lines have been calculated. The plasma parameters used were electron density of 1017 cm−3 and temperature from 5 000 K to 80 000 K. Calculations were performed using the simplified modified semiempirical (SMSE) approach and compared with calculations by Cowley’s approximative Stark broadening formula at 10000 K, usefull in spectrum synthesis. The results have also been considered in the atmosphere model of A type star and for DB white dwarfs.
Ključne reči:
Stark broadening / Spectral lines / Line profilesIzvor:
Advances in Space Research, 2023, 71, 2, 1287-1292Izdavač:
- Elsevier Ltd.
Finansiranje / projekti:
- Ministarstvo nauke, tehnološkog razvoja i inovacija Republike Srbije, institucionalno finansiranje - 200002 (Astronomska opservatorija, Beograd) (RS-200002)
- Ministarstvo nauke, tehnološkog razvoja i inovacija Republike Srbije, institucionalno finansiranje - 200287 (Inovacioni centar Tehnološko-metalurškog fakulteta u Beogradu doo) (RS-200287)
Institucija/grupa
Inovacioni centarTY - JOUR AU - Simić, Zoran AU - Milovanović, Nenad AU - Sakan, Nenad AU - Malović, Miodrag PY - 2023 UR - http://TechnoRep.tmf.bg.ac.rs/handle/123456789/5351 AB - Stark broadening parameters - full widths at half maximum (FWHM) and shifts for 11 Re II lines have been calculated. The plasma parameters used were electron density of 1017 cm−3 and temperature from 5 000 K to 80 000 K. Calculations were performed using the simplified modified semiempirical (SMSE) approach and compared with calculations by Cowley’s approximative Stark broadening formula at 10000 K, usefull in spectrum synthesis. The results have also been considered in the atmosphere model of A type star and for DB white dwarfs. PB - Elsevier Ltd. T2 - Advances in Space Research T1 - On the Stark broadening of the Re II spectral lines EP - 1292 IS - 2 SP - 1287 VL - 71 DO - 10.1016/j.asr.2022.07.079 ER -
@article{ author = "Simić, Zoran and Milovanović, Nenad and Sakan, Nenad and Malović, Miodrag", year = "2023", abstract = "Stark broadening parameters - full widths at half maximum (FWHM) and shifts for 11 Re II lines have been calculated. The plasma parameters used were electron density of 1017 cm−3 and temperature from 5 000 K to 80 000 K. Calculations were performed using the simplified modified semiempirical (SMSE) approach and compared with calculations by Cowley’s approximative Stark broadening formula at 10000 K, usefull in spectrum synthesis. The results have also been considered in the atmosphere model of A type star and for DB white dwarfs.", publisher = "Elsevier Ltd.", journal = "Advances in Space Research", title = "On the Stark broadening of the Re II spectral lines", pages = "1292-1287", number = "2", volume = "71", doi = "10.1016/j.asr.2022.07.079" }
Simić, Z., Milovanović, N., Sakan, N.,& Malović, M.. (2023). On the Stark broadening of the Re II spectral lines. in Advances in Space Research Elsevier Ltd.., 71(2), 1287-1292. https://doi.org/10.1016/j.asr.2022.07.079
Simić Z, Milovanović N, Sakan N, Malović M. On the Stark broadening of the Re II spectral lines. in Advances in Space Research. 2023;71(2):1287-1292. doi:10.1016/j.asr.2022.07.079 .
Simić, Zoran, Milovanović, Nenad, Sakan, Nenad, Malović, Miodrag, "On the Stark broadening of the Re II spectral lines" in Advances in Space Research, 71, no. 2 (2023):1287-1292, https://doi.org/10.1016/j.asr.2022.07.079 . .