Etude du déplacement et du profil de la raie de l'hydrogène Hα aux densités électroniques de l'ordre de 1018 cm-3SALAKHOV, M. KH; SARANDAEV, E. V; LATIPOV, R. Z et al.Optika i spektroskopiâ. 1986, Vol 60, Num 2, pp 431-434, issn 0030-4034Article

The covering factor of quasar broad absorption line cloudsMORRIS, S. L.The Astrophysical journal. 1988, Vol 330, Num 2, pp 83-86, issn 0004-637X, 2Article

Electron-impact shifts of ion lines: modified semiempirical approachDIMITRIJEVIC, M. S; KRSLJANIN, V.Astronomy and astrophysics (Berlin. Print). 1986, Vol 165, Num 1-2, pp 269-274, issn 0004-6361Article

Short term profile variations of three Fe I photospheric lines in solar quiet regions at the disk centerCAVALLINI, F; CEPPATELLI, G; RIGHINI, A et al.Astronomy and astrophysics (Berlin. Print). 1986, Vol 156, Num 1-2, pp 310-314, issn 0004-6361Article

Linear polarization of resonance lines in the absence of magnetic fields. I: Slabs of finite optical thicknessFAUROBERT, M.Astronomy and astrophysics (Berlin. Print). 1987, Vol 178, Num 1-2, pp 269-276, issn 0004-6361Article

On the line emission profile and line source function in the case of partial redistributionFREIRE FERRERO, R.The Astrophysical journal. 1987, Vol 314, Num 2, pp 822-829, issn 0004-637X, 1Article

Fast and accurate generation of the curve of growth for the voigt lineshapeVARDAVAS, I. M.Journal of quantitative spectroscopy & radiative transfer. 1993, Vol 49, Num 2, pp 119-127, issn 0022-4073Article

Non-cosmological redshifts of spectral linesWOLF, E.Nature (London). 1987, Vol 326, Num 6111, pp 363-365, issn 0028-0836Article

A high resolution heterodyne spectrometer from 100 μm to 1000 μm and the detection of CO (J= 7-6), CO (J= 6-5) and ¹³CO (J= 3-2)ROESER, H. P; WATTENBACH, R; DURWEN, E. J et al.Astronomy and astrophysics (Berlin. Print). 1986, Vol 165, Num 1-2, pp 287-299, issn 0004-6361Article

The half-widths of Bragg intensity profiles measured with a triple-crystal diffractometer at a synchrotron-radiation source. I: Derivation of a simple expression for the full width at half-maximumROSSMANITH, E.Journal of applied crystallography. 1993, Vol 26, pp 753-755, issn 0021-8898, 6Article

Stark shifts of singly-ionized nitrogen spectral linesDJENIZE, S; SRECKOVIC, A; LABAT, J et al.Astronomy and astrophysics (Berlin. Print). 1992, Vol 253, Num 2, pp 632-634, issn 0004-6361Article

Broad-line variability in NGC 5548KALLMAN, T; ELITZUR, M.The Astrophysical journal. 1988, Vol 328, Num 2, pp 523-529, issn 0004-637X, 1Article

Non-LTE line formation in early B and late O stars. II: Equivalent widths for O IIBECKER, S. R; BUTLER, K.Astronomy & astrophysics. Supplement Series (Print). 1988, Vol 74, Num 2, pp 211-225, issn 0365-0138Article

Profile variations of some photospheric lines as observed in active regions across the solar diskCAVALLINI, F; CEPPATELLI, G; RIGHINI, A et al.Astronomy and astrophysics (Berlin. Print). 1988, Vol 205, Num 1-2, pp 278-288, issn 0004-6361Article

Simple formulae for estimating Stark widths and shifts of neutral atom linesDIMITRIJEVIC, M. S; KONJEVIC, N.Astronomy and astrophysics (Berlin. Print). 1986, Vol 163, Num 1-2, pp 297-300, issn 0004-6361Article

Classification of mathematical models of peak-shaped analytical signalsROMANENKO, S. V; STROMBERG, A. G.Journal of analytical chemistry (New York, NY). 2000, Vol 55, Num 11, pp 1024-1028, issn 1061-9348Article

Mg I as a probe of the solar chromosphere: the atomic modelMAUAS, P. J; AVRETT, E. H; LOESER, R et al.The Astrophysical journal. 1988, Vol 330, Num 2, pp 1008-1021, issn 0004-637X, 1Article

Half-width, shift and transition probability of Ar II linesABBAS, A; BASHA, T. S; ABDEL-AAL, Z. A et al.Japanese journal of applied physics. 1988, Vol 27, Num 5, pp 804-807, issn 0021-4922, 1Article

The Stark broadening of the He I 667.8 nm lineVUJICIC, B. T; DJUROVIC, S; HALENKA, J et al.Zeitschrift für Physik. D, atoms, molecules and clusters. 1989, Vol 11, Num 2, pp 119-121, issn 0178-7683Article

Noble gas line profiles in dense plasmas. I: ArgonVITEL, Y; SKOWRONEK, M.Journal of physics. B. Atomic and molecular physics. 1987, Vol 20, Num 24, pp 6477-6491, issn 0022-3700Article

Noble gas line profiles in dense plasmas. II: Krypton and xenonVITEL, Y; SKOWRONEK, M.Journal of physics. B. Atomic and molecular physics. 1987, Vol 20, Num 24, pp 6493-6506, issn 0022-3700Article

On the origin of penumbral line asymmetriesDEGENHARDT, D.Astronomy and astrophysics (Berlin. Print). 1993, Vol 277, Num 1, pp 235-241, issn 0004-6361Article

Widths and shifts of some plasma-broadened oxygen and carbon multipletsGOLY, A; WENIGER, S.Journal of quantitative spectroscopy & radiative transfer. 1987, Vol 38, Num 3, pp 225-230, issn 0022-4073Article

Dépendance de demi-largeurs et largeurs équivalentes observées du fer neutre dans le spectre solaire sur le potentiel d'excitationBABIJ, B. T.Pis′ma v Astronomičeskij žurnal. 1988, Vol 14, Num 4, pp 353-356, issn 0320-0108Article

Fine-structure population ratios for the ²P ground state of C IIKEENAN, F. P; LENNON, D. J; JOHNSON, C. T et al.Monthly Notices of the Royal Astronomical Society. 1986, Vol 220, Num 2, pp 571-576, issn 0035-8711Article