Results 21 to 30 of about 786 (162)
Atoms, 2019 Calculated radiative transition probabilities and oscillator strengths are reported for 392 lines of neutral lanthanum (La I) atom in the spectral range from the near ultraviolet to the mid infrared.
Sébastien Gamrath +2 more
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Current Status and Developments of the Atomic Database on Rare-Earths at Mons University (DREAM)
Atoms, 2020 The main purpose of the Database on Rare Earths At Mons University (DREAM) is to provide the scientific community with updated spectroscopic parameters related to lanthanide atoms (Z = 57–71) in their lowest ionization stages.
Pascal Quinet, Patrick Palmeri
doaj +1 more source
Stark broadening parameter tables for Ar VIII [PDF]
Serbian Astronomical Journal, 1999 Using a semiclassical approach, we have calculated electron−, proton−, and He III−impact line widths and shifts for 9 Ar VIII transitions as a function of temperature and perturber density.
Dimitrijević M.S., Sahal−Bréchot S.
doaj +1 more source
Stark broadening parameter tables for Kr VIII [PDF]
Serbian Astronomical Journal, 1999 Using a semiclassical approach, we have calculated electron−, proton−, and He III−impact line widths and shifts for 6 Kr VIII multiplets as a function of temperature and perturber density.
Dimitrijević M.S., Sahal−Bréchot S.
doaj +1 more source
Use of the ESI-2007 scale to evaluate the 2003 Boumerdès earthquake (North Algeria)
Annals of Geophysics, 2016 In this study, we applied the environmental seismic intensity (ESI-2007) scale to a major recent Algerian earthquake. The ESI-2007 scale is an effective tool to assess the seismic hazard and has been applied to onshore earthquakes.
Aicha Heddar +5 more
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Stark broadening parameter tables for Na X [PDF]
Serbian Astronomical Journal, 1998 Using a semiclassical approach, we have calculated electron−, proton−, and He III−impact line widths and shifts for 57 Na X multiplets as a function of temperature (200 000 K - 5 000 000 K) and perturber density (1017cm−3 - 1024cm−3.
Dimitrijević M.S., Sahal−Bréchot S.
doaj +1 more source
Stark broadening parameter tables for in II: Part II [PDF]
Serbian Astronomical Journal, 2001 Electron-, proton-, and ionized helium-impact broadening parameter tables for 101 In II multiplets, are presented as a function of temperature for the perturber density of 1016cm-3.
Dimitrijević M.S., Sahal-Brechot S.
doaj +1 more source
Stark broadening parameter tables for K VIII and K IX [PDF]
Serbian Astronomical Journal, 1998 Using a semiclassical approach, we have calculated electron−, proton−, and He III−impact line widths and shifts for 4 K VIII and 30 K IX multiplets as a function of temperature and perturber density.
Dimitrijević M.S., Sahal−Bréchot S.
doaj +1 more source
La physique nucléaire en astrophysique [PDF]
Annales de Physique, 2001 L'astrophysique nucleaire est sans nul doute l'une des branches les plus largement interdisciplinaires de la science et est intimement connectee a une tres grande variete d'autres domaines de recherche. Cet ouvrage se limite a une breve presentation des relations privilegiees qui se sont etablies entre l'astrophysique et la physique nucleaire.
Arnould, Marcel, Samyn, Mathieu
openaire +1 more source
Atoms, 2015 A new set of oscillator strengths and transition probabilities for EUV spectral lines of seven times ionized tungsten (W VIII) is reported in the present paper.
Jérôme Deprince, Pascal Quinet
doaj +1 more source