Stark Broadening in Compact Stars: Xe VI Lines
Само за регистроване кориснике
2015
Аутори
Dimitrijević, Milan S.Simić, Zoran
Kovačević, Anđelka
Valjarević, Aleksandar
Sahal-Brechot, Sylvie
Конференцијски прилог (Објављена верзија)
Метаподаци
Приказ свих података о документуАпстракт
We will consider Stark broadening of non hydrogenic spectral lines in the impact approximation in compact stars: pre-white dwarf and white dwarf atmospheres. In order to show an example, Stark broadening parameters have been calculated, using the impact semiclassical perturbation approach for four Xe VI spectral lines. Obtained results have been used to demonstrate the influence of Stark broadening in DA and DB white dwarf atmospheres.
Кључне речи:
Stark broadening / atomic data / white dwarfs / Xe VIИзвор:
Journal of Astrophysics and Astronomy, 2015, 36, 4, 681-691Издавач:
- Indian Acad Sciences, Bangalore
Финансирање / пројекти:
- Утицај судара на спектре астрофизичке плазме (RS-MESTD-Basic Research (BR or ON)-176002)
- Paris Observatory
- Centre National de la Recherche Scientifique (CNRS) - European Commission
- PNPS (Programme National de Physique Stellaire, INSU-CNRS)
- Investissements d'avenir, French National Research Agency (ANR) [ANR-11-IDEX-0004-02]
DOI: 10.1007/s12036-015-9352-y
ISSN: 0250-6335
WoS: 000368698700023
Scopus: 2-s2.0-84956613605
Колекције
Институција/група
Geografski fakultetTY - CONF AU - Dimitrijević, Milan S. AU - Simić, Zoran AU - Kovačević, Anđelka AU - Valjarević, Aleksandar AU - Sahal-Brechot, Sylvie PY - 2015 UR - https://gery.gef.bg.ac.rs/handle/123456789/728 AB - We will consider Stark broadening of non hydrogenic spectral lines in the impact approximation in compact stars: pre-white dwarf and white dwarf atmospheres. In order to show an example, Stark broadening parameters have been calculated, using the impact semiclassical perturbation approach for four Xe VI spectral lines. Obtained results have been used to demonstrate the influence of Stark broadening in DA and DB white dwarf atmospheres. PB - Indian Acad Sciences, Bangalore C3 - Journal of Astrophysics and Astronomy T1 - Stark Broadening in Compact Stars: Xe VI Lines VL - 36 IS - 4 SP - 681 EP - 691 DO - 10.1007/s12036-015-9352-y UR - https://hdl.handle.net/21.15107/rcub_gery_728 ER -
@conference{ author = "Dimitrijević, Milan S. and Simić, Zoran and Kovačević, Anđelka and Valjarević, Aleksandar and Sahal-Brechot, Sylvie", year = "2015", abstract = "We will consider Stark broadening of non hydrogenic spectral lines in the impact approximation in compact stars: pre-white dwarf and white dwarf atmospheres. In order to show an example, Stark broadening parameters have been calculated, using the impact semiclassical perturbation approach for four Xe VI spectral lines. Obtained results have been used to demonstrate the influence of Stark broadening in DA and DB white dwarf atmospheres.", publisher = "Indian Acad Sciences, Bangalore", journal = "Journal of Astrophysics and Astronomy", title = "Stark Broadening in Compact Stars: Xe VI Lines", volume = "36", number = "4", pages = "681-691", doi = "10.1007/s12036-015-9352-y", url = "https://hdl.handle.net/21.15107/rcub_gery_728" }
Dimitrijević, M. S., Simić, Z., Kovačević, A., Valjarević, A.,& Sahal-Brechot, S.. (2015). Stark Broadening in Compact Stars: Xe VI Lines. in Journal of Astrophysics and Astronomy Indian Acad Sciences, Bangalore., 36(4), 681-691. https://doi.org/10.1007/s12036-015-9352-y https://hdl.handle.net/21.15107/rcub_gery_728
Dimitrijević MS, Simić Z, Kovačević A, Valjarević A, Sahal-Brechot S. Stark Broadening in Compact Stars: Xe VI Lines. in Journal of Astrophysics and Astronomy. 2015;36(4):681-691. doi:10.1007/s12036-015-9352-y https://hdl.handle.net/21.15107/rcub_gery_728 .
Dimitrijević, Milan S., Simić, Zoran, Kovačević, Anđelka, Valjarević, Aleksandar, Sahal-Brechot, Sylvie, "Stark Broadening in Compact Stars: Xe VI Lines" in Journal of Astrophysics and Astronomy, 36, no. 4 (2015):681-691, https://doi.org/10.1007/s12036-015-9352-y ., https://hdl.handle.net/21.15107/rcub_gery_728 .