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Excitation mechanisms and characterization of a multi-ionic xenon laser
(Centro de Investigaciones Ópticas (CIOP), 1999)
Modified branching ratio method for absolute intensity calibration in VUV spectroscopy
(Ieee-inst Electrical Electronics Engineers IncPiscatawayEUA, 2005)
Generalised collisional-radiative model for light elements. A: Data for the Li isonuclear sequence
(Elsevier, 2006-12)
A first stage collision database is assembled which contains electron-impact effective collision strengths, and ionization and recombination rate coefficients for Li, Li+, and Li2+. The first stage database is constructed ...
Dirac R--matrix calculations of electron--impact excitation of neon--like krypton
(IOP Publishing, 2008-12)
We have employed the Dirac R-matrix method to determine electron-impact excitation cross sections and effective collision strengths in Ne-like Kr26+. Both the configuration-interaction expansion of the target and the ...
Hydrodynamical interaction of stellar and planetary winds: Effects of charge exchange and radiation pressure on the observed Ly α absorption
(Wiley Blackwell Publishing, Inc, 2019-06)
Lyman α observations of the transiting exoplanet HD 209458b enable the study of exoplanet exospheres exposed to stellar extreme ultraviolet (EUV) fluxes, as well as the interacting stellar wind properties. In this study ...
Numerical modeling of magnetospheric electron radial transport with accounting synchrotron radiation losses
(Amer Geophysical UnionWashingtonEUA, 1998)
Radiation thermo-chemical models of protoplanetary discs IV. Modelling CO ro-vibrational emission from Herbig Ae discs
(EDP Sciences, 2013)
Context. The carbon monoxide (CO) ro-vibrational emission from discs around Herbig Ae stars and T Tauri stars with strong ultraviolet
emissions suggests that fluorescence pumping from the ground X1Σ+ to the electronic A1Π ...
Planck intermediate results. XV. A study of anomalous microwave emission in Galactic clouds
(European Southern Observatory., 2014-05-20)
Anomalous microwave emission (AME) is believed to be due to electric dipole radiation from small spinning dust grains. The aim of this paper is
a statistical study of the basic properties of AME regions and the environment ...
Aquecimento em colunas de acreção de estrelas T Tauri
(Universidade Federal de Minas GeraisUFMG, 2011-03-02)
Young low mass stars that show signs of accretion, the classical T Tauri stars (CTTSs), present a significant number of emission lines in their spectra. These emission lines, thought to be produced in accretion columns, ...