Выдержка
Elementary processes in astrophysical environments traditionally attract researchers' attention. We present the data needed for the inclusion of the specific atomic collisional processes in the investigation of the optical and kinetic properties of weakly ionized stellar atmosphere layers. The first type of processes are collisional ionisation (chemi-ionization) processes, and the second ones are excitation and de-excitation (i.e., (n - n')-mixing processes). We give the rate coefficients of the aforementioned processes for the conditions that exist in the solar photosphere, the atmosphere of DB white dwarfs, M-type red dwarfs, etc.
| Язык оригинала | английский |
|---|---|
| Номер статьи | 72 |
| Журнал | Galaxies |
| Том | 6 |
| Номер выпуска | 3 |
| DOI | |
| Состояние | Опубликовано - 16 июл 2018 |
Отпечаток
Предметные области Scopus
- Астрономия и астрофизика
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The collisional atomic processes of rydberg hydrogen and helium atoms : Astrophysical relevance. / Sreçkoviç, Vladimir A.; Dimitrijeviç, Milan S.; Ignjatoviç, Ljubinko M.; Bezuglov, Nikolai N.; Klyucharev, Andrey N.
В: Galaxies, Том 6, № 3, 72, 16.07.2018.Результат исследований: Научные публикации в периодических изданиях › статья
TY - JOUR
T1 - The collisional atomic processes of rydberg hydrogen and helium atoms
T2 - Astrophysical relevance
AU - Sreçkoviç, Vladimir A.
AU - Dimitrijeviç, Milan S.
AU - Ignjatoviç, Ljubinko M.
AU - Bezuglov, Nikolai N.
AU - Klyucharev, Andrey N.
PY - 2018/7/16
Y1 - 2018/7/16
N2 - Elementary processes in astrophysical environments traditionally attract researchers' attention. We present the data needed for the inclusion of the specific atomic collisional processes in the investigation of the optical and kinetic properties of weakly ionized stellar atmosphere layers. The first type of processes are collisional ionisation (chemi-ionization) processes, and the second ones are excitation and de-excitation (i.e., (n - n')-mixing processes). We give the rate coefficients of the aforementioned processes for the conditions that exist in the solar photosphere, the atmosphere of DB white dwarfs, M-type red dwarfs, etc.
AB - Elementary processes in astrophysical environments traditionally attract researchers' attention. We present the data needed for the inclusion of the specific atomic collisional processes in the investigation of the optical and kinetic properties of weakly ionized stellar atmosphere layers. The first type of processes are collisional ionisation (chemi-ionization) processes, and the second ones are excitation and de-excitation (i.e., (n - n')-mixing processes). We give the rate coefficients of the aforementioned processes for the conditions that exist in the solar photosphere, the atmosphere of DB white dwarfs, M-type red dwarfs, etc.
KW - Atomic and molecular databases
KW - Atomic data
KW - Molecular data
UR - http://www.scopus.com/inward/record.url?scp=85051491449&partnerID=8YFLogxK
U2 - 10.3390/galaxies6030072
DO - 10.3390/galaxies6030072
M3 - Article
AN - SCOPUS:85051491449
VL - 6
JO - Galaxies
JF - Galaxies
SN - 2075-4434
IS - 3
M1 - 72
ER -