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Formation of ZrI and II Lines under Non-LTE Conditions of Stellar AtmospheresVELICHKO, A. B; MASHONKINA, L. I; NILSSON, H et al.Astronomy letters (Print). 2010, Vol 36, Num 9, pp 664-679, issn 1063-7737, 16 p.Article

Two-dimensional radiative transfer with partial frequency redistribution. I: General methodAUER, L. H; PALETOU, F.Astronomy and astrophysics (Berlin. Print). 1994, Vol 285, Num 2, pp 675-686, issn 0004-6361Article

Hydrodynamics and multi-level non-LTE radiative transfer in pulsating atmospheres: CepheidsSASSELOV, D. D.Astrophysics and space science. 1993, Vol 210, Num 1-2, pp 329-330, issn 0004-640XConference Paper

NLTE model stellar atmospheres with line blanketing near the series limitsHUBENY, I; HUMMER, D. G; LANZ, T et al.Astronomy and astrophysics (Berlin. Print). 1994, Vol 282, Num 1, pp 151-167, issn 0004-6361Article

Superheat turbulence in gas discharged plasmaLEVITAN, Y. S.IEEE transactions on plasma science. 1993, Vol 21, Num 6, pp 614-618, issn 0093-3813Article

The use of iteration factors in the solution of the NLTE line transfer problem. I: Two-level atomATANACKOVIC-VUKMANOVIC, O; SIMONNEAU, E.Journal of quantitative spectroscopy & radiative transfer. 1994, Vol 51, Num 3, pp 525-543, issn 0022-4073Article

Three-dimensional radiative transfer on a massively parallel computerVATH, H. M.Astronomy and astrophysics (Berlin. Print). 1994, Vol 284, Num 1, pp 319-330, issn 0004-6361Article

Direct evidence of departure from local thermodynamic equilibrium in a free-burning arc-discharge plasmaSNYDER, S. C; LASSAHN, G. D; REYNOLDS, L. D et al.Physical review. A. 1993, Vol 48, Num 5, pp 4124-4127, issn 1050-2947, EArticle

Radiative equilibrium in solar prominences reconsideredHEINZEL, P; ANZER, U.Astronomy and astrophysics (Berlin. Print). 2012, Vol 539, issn 0004-6361, A49.1-A49.6, 1Article

Non-lte monte carlo radiative transfer. I. The thermal properties of keplerian disks around classical be starsCARCIOFI, A. C; BJORKMAN, J. E.The Astrophysical journal. 2006, Vol 639, Num 2, pp 1081-1094, issn 0004-637X, 14 p., 1Article

On the neon abundance in PG 1159-type central stars of planetary nebulaeWERNER, K; RAUCH, T.Astronomy and astrophysics (Berlin. Print). 1994, Vol 284, Num 1, pp L5-L8, issn 0004-6361Article

Radiation-driven winds of hot luminous stars. XII: A first step towards detailed UV-line diagnostics of O-starsPAULDRACH, A. W. A; KUDRITZKI, R. P; PULS, J et al.Astronomy and astrophysics (Berlin. Print). 1994, Vol 283, Num 2, pp 525-560, issn 0004-6361Article

Non-lte spectra of accretion disks around intermediate-mass black holesYAWEI HUI; KROLIK, Julian H; HUBENY, Ivan et al.The Astrophysical journal. 2005, Vol 625, Num 2, pp 913-922, issn 0004-637X, 10 p., 1Article

High-resolution observations of Martian non-thermal CO2 emission near 10μm with a new tuneable heterodyne receiverSONNABEND, G; WIRTZ, D; VETTERLE, V et al.Astronomy and astrophysics (Berlin. Print). 2005, Vol 435, Num 3, pp 1181-1184, issn 0004-6361, 4 p.Article

Analysis of the DA white dwarf HZ 43 A and its companion starNAPIWOTZKI, R; BARSTOW, M. A; FLEMING, T et al.Astronomy and astrophysics (Berlin. Print). 1993, Vol 278, Num 2, pp 478-486, issn 0004-6361Article

NLTE analysis of hot binariesSIMON, K. P; STURM, E.Space science reviews. 1993, Vol 66, Num 1-4, pp 199-202, issn 0038-6308Conference Paper

C2H in prestellar coresPADOVANI, M; WALMSLEY, C. M; TAFALLA, M et al.Astronomy and astrophysics (Berlin. Print). 2009, Vol 505, Num 3, pp 1199-1211, issn 0004-6361, 13 p.Article

An implicit integral method to solve selected radiative transfer problems. I: Non-LTE line formationSIMONNEAU, E; CRIVELARI, L.The Astrophysical journal. 1993, Vol 409, Num 2, pp 830-840, issn 0004-637X, 1Article

NON-LTE MODELING OF THE NEAR-ULTRAVIOLET BAND OF LATE-TYPE STARSSHORT, C. Ian; HAUSCHILDT, P. H.The Astrophysical journal. 2009, Vol 691, Num 2, pp 1634-1647, issn 0004-637X, 14 p., 1Article

Properties of prominence fine-structure threads derived from SOHO/SUMER hydrogen Lyman linesGUNAR, S; HEINZEL, P; SCHMIEDER, B et al.Astronomy and astrophysics (Berlin. Print). 2007, Vol 472, Num 3, pp 929-936, issn 0004-6361, 8 p.Article

Phénomènes radiatifs dans des atmosphères stellaires étendues: application à la formation des raies en émission dans les variables à longue période = Radiative processes in extended stellar atmospheres: application to the formation of emission lines in long-period variablesDe Laverny, Patrick; Magnan, C.1994, 223 p.Thesis

Non-LTE analyses of neutral nitrogen lines in two supergiants: alpha Cygni and beta OrionisSADAKANE, K; TAKEDA, Y; OKYUDO, M et al.Publications of the Astronomical Society of Japan. 1993, Vol 45, Num 3, pp 471-476, issn 0004-6264Article

LTE and NLTE abundances in A-supergiants a test of their evolutionary statusVENN, K. A.Space science reviews. 1993, Vol 66, Num 1-4, pp 163-168, issn 0038-6308Conference Paper

Line blanketed non-LTE atmosphere models for Wolf-Rayet starsSCHMUTZ, W.Space science reviews. 1993, Vol 66, Num 1-4, pp 253-261, issn 0038-6308Conference Paper

ARGON ABUNDANCES IN THE SOLAR NEIGHBORHOOD : NON-LTE ANALYSIS OF ORION ASSOCIATION B-TYPE STARSLANZ, Thierry; CUNHA, Katia; HOLTZMAN, Jon et al.The Astrophysical journal. 2008, Vol 678, Num 2, pp 1342-1350, issn 0004-637X, 9 p., 1Article

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