On the Stark broadening of the Re II spectral lines
Само за регистроване кориснике
2023
Чланак у часопису (Објављена верзија)
Метаподаци
Приказ свих података о документуАпстракт
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.
Кључне речи:
Stark broadening / Spectral lines / Line profilesИзвор:
Advances in Space Research, 2023, 71, 2, 1287-1292Издавач:
- Elsevier Ltd.
Финансирање / пројекти:
- Министарство науке, технолошког развоја и иновација Републике Србије, институционално финансирање - 200002 (Астрономска опсерваторија, Београд) (RS-MESTD-inst-2020-200002)
- Министарство науке, технолошког развоја и иновација Републике Србије, институционално финансирање - 200287 (Иновациони центар Технолошко-металуршког факултета у Београду доо) (RS-MESTD-inst-2020-200287)
Институција/група
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 . .