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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.

In: Galaxies, Vol. 6, No. 3, 72, 16.07.2018.

Research output: Contribution to journal › Article › peer-review

Harvard

Sreçkoviç, VA, Dimitrijeviç, MS, Ignjatoviç, LM, Bezuglov, NN & Klyucharev, AN 2018, 'The collisional atomic processes of rydberg hydrogen and helium atoms: Astrophysical relevance', Galaxies, vol. 6, no. 3, 72. https://doi.org/10.3390/galaxies6030072

APA

Sreçkoviç, V. A., Dimitrijeviç, M. S., Ignjatoviç, L. M., Bezuglov, N. N., & Klyucharev, A. N. (2018). The collisional atomic processes of rydberg hydrogen and helium atoms: Astrophysical relevance. Galaxies, 6(3), [72]. https://doi.org/10.3390/galaxies6030072

Vancouver

Sreçkoviç VA, Dimitrijeviç MS, Ignjatoviç LM, Bezuglov NN, Klyucharev AN. The collisional atomic processes of rydberg hydrogen and helium atoms: Astrophysical relevance. Galaxies. 2018 Jul 16;6(3). 72. https://doi.org/10.3390/galaxies6030072

Author

Sreçkoviç, Vladimir A. ; Dimitrijeviç, Milan S. ; Ignjatoviç, Ljubinko M. ; Bezuglov, Nikolai N. ; Klyucharev, Andrey N. / The collisional atomic processes of rydberg hydrogen and helium atoms : Astrophysical relevance. In: Galaxies. 2018 ; Vol. 6, No. 3.

BibTeX

@article{92ac362897764f3eba3a83ea9b2cf23b,
title = "The collisional atomic processes of rydberg hydrogen and helium atoms: Astrophysical relevance",
abstract = "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.",
keywords = "Atomic and molecular databases, Atomic data, Molecular data, STATE, CHEMI-RECOMBINATION PROCESSES, PLASMA, atomic data, molecular data, ABSORPTION, SPECTRA, IONIZATION PROCESSES, atomic and molecular databases, LINE FORMATION",
author = "Sre{\c c}kovi{\c c}, {Vladimir A.} and Dimitrijevi{\c c}, {Milan S.} and Ignjatovi{\c c}, {Ljubinko M.} and Bezuglov, {Nikolai N.} and Klyucharev, {Andrey N.}",
year = "2018",
month = jul,
day = "16",
doi = "10.3390/galaxies6030072",
language = "English",
volume = "6",
journal = "Galaxies",
issn = "2075-4434",
publisher = "MDPI AG",
number = "3",

}

RIS

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

KW - STATE

KW - CHEMI-RECOMBINATION PROCESSES

KW - PLASMA

KW - atomic data

KW - molecular data

KW - ABSORPTION

KW - SPECTRA

KW - IONIZATION PROCESSES

KW - atomic and molecular databases

KW - LINE FORMATION

UR - http://www.scopus.com/inward/record.url?scp=85051491449&partnerID=8YFLogxK

UR - http://www.mendeley.com/research/collisional-atomic-processes-rydberg-hydrogen-helium-atoms-astrophysical-relevance

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 -

ID: 36429466