Zobrazeno 1 - 10
of 780
pro vyhledávání: '"Zatsarinny, A. A."'
Publikováno v:
J. Chem. Phys. 158, 134306 (2023)
A decade ago, an electron-attachment process called interatomic Coulombic electron capture has been predicted to be possible through energy transfer to a nearby neighbor. It has been estimated to be competitive with environment-independent photorecom
Externí odkaz:
http://arxiv.org/abs/2306.11738
We present accurate element abundance patterns based on the non-local thermodynamic equilibrium (non-LTE, NLTE) line formation for 14 chemical elements from He to Nd for a sample of nine A9 to B3 type stars with well determined atmospheric parameters
Externí odkaz:
http://arxiv.org/abs/2010.02058
Autor:
Schneider, Barry I., Klaus~Bartschat, Zatsarinny, Oleg, Bray, Igor, Scrinzi, Armin, Martin, Fernando, Klinker, Markus, Tennyson, Jonathan, Gorfinkiel, Jimena D., Pamidighantam, Sudhakar
We describe the creation of a new Atomic and Molecular Physics science gateway (AMPGateway). The gateway is designed to bring together a subset of the AMP community to work collectively to make their codes available and easier to use by the partners
Externí odkaz:
http://arxiv.org/abs/2001.02286
Autor:
Reggiani, Henrique, Amarsi, Anish M., Lind, Karin, Barklem, Paul S., Zatsarinny, Oleg, Bartschat, Klaus, Fursa, Dmitry V., Bray, Igor, Spina, Lorenzo, Meléndez, Jorge
Publikováno v:
A&A 627, A177 (2019)
Older GCE models predict [K/Fe] ratios as much as 1 dex lower than those inferred from stellar observations. Abundances of potassium are mainly based on analyses of the 7698 $\AA$ resonance line, and the discrepancy between models and observations is
Externí odkaz:
http://arxiv.org/abs/1906.08281
Publikováno v:
A&A 623, A103 (2019)
Context. Departures from local thermodynamic equilibrium (LTE) distort the calcium abundance derived from stellar spectra in various ways, depending on the lines used and the stellar atmospheric parameters. The collection of atomic data adopted in no
Externí odkaz:
http://arxiv.org/abs/1901.11442
Publikováno v:
Phys. Rev. A 99, 012706 (2019)
We present a comprehensive study of electron collisions with calcium atoms by using the convergent \emph{B}-spline \emph{R}-matrix method. Elastic, excitation, and ionization cross sections were obtained for all transitions between the lowest 39 phys
Externí odkaz:
http://arxiv.org/abs/1811.07176
Publikováno v:
A&A 616, A89 (2018)
The OI 777 nm triplet is a key diagnostic of oxygen abundances in the atmospheres of FGK-type stars; however it is sensitive to departures from local thermodynamic equilibrium (LTE). The accuracy of non-LTE line formation calculations has hitherto be
Externí odkaz:
http://arxiv.org/abs/1803.10531
Autor:
Barklem, P. S., Osorio, Y., Fursa, D. V., Bray, I., Zatsarinny, O., Bartschat, K., Jerkstrand, A.
Publikováno v:
A&A 606, A11 (2017)
Results of calculations for inelastic e+Mg effective collision strengths for the lowest 25 physical states of Mg I (up to 3s6p 1P), and thus 300 transitions, from the convergent close-coupling (CCC) and the B-spline R-matrix (BSR) methods are present
Externí odkaz:
http://arxiv.org/abs/1706.03399
Publikováno v:
Phys. Rev. A 95, 042709 (2017)
There are major discrepancies between recent B-spline R-matrix (BSR) and Dirac Atomic R-matrix Code (DARC) calculations regarding electron-impact excitation rates for transitions in Mg$^{4+}$, with claims that the DARC calculations are much more accu
Externí odkaz:
http://arxiv.org/abs/1701.08207
Publikováno v:
J Phys B: AMOP. 50: 065203 (2017)
There are major discrepancies between recent ICFT (Intermediate Coupling Frame Transformation) and DARC (Dirac Atomic R-matrix Code) calculations (Fern\'andez-Menchero et al. 2014, Astron. Astroph. 566 A104, Aggarwal et al. 2016 Mon. Not. R Astr. Soc
Externí odkaz:
http://arxiv.org/abs/1611.04657