THE ELECTRON TEMPERATURES OF THE (O III) ZONE OF M₄₂.GIBBONS AH.1976; MONTH. NOT. R. ASTR. SOC.; G.B.; DA. 1976; VOL. 174; NO 1; PP. 105-109; BIBL. 6 REF.Article

LINE PROFILES AND MAGNETIC INTENSIFICATION IN MAGNETIC STARS.HAVNES O; MOE OK.1975; ASTR. AND ASTROPHYS.; GERM.; DA. 1975; VOL. 42; NO 2; PP. 269-272; BIBL. 9 REF.Article

MESURE DES CONTOURS DE RAIES PAR LES TECHNIQUES DE TELEVISION.FEHRENBACH C; VIN A.1975; ASTROPHYS. SPACE SCI. LIBRARY; NETHERL.; DA. 1975; VOL. 54; PP. 109-116; (IMAGE PROCESS. TECH. ASTRON. PROC. CONF.; UTRECHT; 1975)Conference Paper

SOLAR LINE PROFILES OF HE I 584 A AND HE II 304 A.CUSHMAN GW; FARWELL L; GODDEN G et al.1975; J. GEOPHYS. RES.; U.S.A.; DA. 1975; VOL. 80; NO 4; PP. 482-486; BIBL. 11 REF.Article

DISTRIBUTION DES DEMI-LARGEURS DES PROFILS DES RAIES CORONALESTETRUASHVILI EH I.1975; ABASTUMAN. ASTROFIZ. OBS., BJULL.; S.S.S.R.; DA. 1975; NO 46; PP. 185-188; ABS. GEORGIEN ANGL.; BIBL. 5 REF.Article

POSSIBILITES ET RESTRICTIONS DE LA METHODE DE "CARTOGRAPHIE" DE LA SURFACE DES ETOILES AP D'APRES LES PROFILS DES RAIES SPECTRALESKHOKHLOVA VL.1975; ASTR. ZH.; S.S.S.R.; DA. 1975; VOL. 52; NO 5; PP. 950-955; BIBL. 7 REF.Article

SPLITTINGS IN QUASAR ABSORPTION LINES.BAHCALL JN.1975; ASTROPHYS. J.; U.S.A.; DA. 1975; VOL. 200; NO 1 PART. 2; PP. L1-L3; BIBL. 27 REF.Article

LA PRISE EN COMPTE DES INHOMOGENEITES DES OBJETS POUR LE CALCUL DES PROFILS DE RAIESKUROCHKA LN; OSTAPENKO VA.1975; SOLNECH. DANNYE, BJULL.; S.S.S.R.; DA. 1975; NO 7; PP. 96-102; ABS. ANGL.; BIBL. 8 REF.Article

ELECTRON SCATTERING IN SPHERICALLY EXPANDING ENVELOPESAUER LH; VAN BLERKOM D.1972; ASTROPHYS. J.,; U.S.A.; DA. 1972; VOL. 178; NO 1, PART1; PP. 175-181; BIBL. 12REF.Serial Issue

THE HELIUM 10830 A LINE IN EARLY-TYPE STARS; AN ATLAS OF FABRY-PEROT SCANSMEISEL DD; SAUNDERS BA; FRANK ZA et al.1982; ASTROPHYSICAL JOURNAL; ISSN 0004-637X; USA; DA. 1982; VOL. 263; NO 2; PART. 1; PP. 759-776; BIBL. 63 REF.Article

A MECHANISM FOR THE PRODUCTION OF LIGHT AND DARK CONTRASTS IN RADIATIVELY CONTROLLED LINESGEBBIE KB; STEINITZ R.1973; SOLAR PHYS.; NETHERL.; DA. 1973; VOL. 29; NO 1; PP. 3-15; BIBL. 4 REF.Serial Issue

OBSERVATIONS OF SHIFTS OF HYDROGEN LINESBENGTSON RD; CHESTER GR.1972; ASTROPHYS. J.,; U.S.A.; DA. 1972; VOL. 178; NO 2PART1; PP. 565-569; BIBL. 13REF.Serial Issue

PROFILS ET LARGEURS A MI HAUTEUR DES RAIES TELLURIQUESKOZHEVNIKOV NI; SITNIK GF; KHLYSTOV AI et al.1972; SOOBSHCH. GOS. ASTR. INST. P.K. SHTERNBERGA; S.S.S.R.; DA. 1972; NO 180; PP. 3-19; ABS. ANGL; BIBL. 15REF.Serial Issue

ANALYSE DES PROFILS DES RAIES MAGNETOACTIVES. II. LARGEURS EQUIVALENTES ET DEGRES DE POLARISATION CIRCULAIRE DES RAIESBARANOV AV.1975; SOLNECH. DANNYE, BJULL.; S.S.S.R.; DA. 1975; NO 2; PP. 52-55; ABS. ANGL.; BIBL. 3 REF.Article

THE WIDTHS OF THE SOLAR HE I AND HE II LINES AT 584, 537, AND 304 A.DOSCHEK GA; BEHRING WE; FELDMAN U et al.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 190; NO 3 PART. 2; PP. 141-142; BIBL. 13 REF.Article

TRANSFER OF LINE RADIATION IN DIFFERENTIALLY EXPANDING ATMOSPHERES, IV. THE TWO-LEVEL ATOM IN PLANE PARALLEL GEOMETRY SOLVED BY THE FEAUTRIER METHOD.NOERDLINGER PD; RYBICKI GB.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 193; NO 3 PART. 1; PP. 651-676; BIBL. 23 REF.Article

DETERMINATION DES PROFILS VRAIS DES RAIES DE FRAUNHOFER DANS LE SPECTRE SOLAIREPECHINSKAYA NI.1974; SOLNECH DANNYE, BJULL.; S.S.S.R.; DA. 1974; NO 10; PP. 85-93; ABS. ANGL.; BIBL. 18 REF.Article

MAGNESIUMII DOUBLET PROFILES OF CHROMOSPHERIC INHOMOGENEITIES AT THE CENTER OF THE SOLAR DISKLEMAIRE P; SKUMANICH A.1973; ASTR. AND ASTROPHYS.,; GERM.; DA. 1973; VOL. 22; NO 1; PP. 61-68; BIBL. 28REF.Serial Issue

ON THE DEPENDENCE OF THE TWO-LEVEL SOURCE FUNCTION ON ITS OWN RADIATION FIELDSTEINITZ R; SHINE RA.1973; MONTH. NOT. ASTR. SOC.; G.B.; DA. 1973; VOL. 162; NO 3; PP. 197-206; BIBL. 9REF.Serial Issue

SOME OBSERVATIONAL CONSEQUENCES OF RESIDUAL HI IN GALACTIC MOLECULAR CLOUDSLISZT HS; BURTON WB; BANIA TM et al.1981; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1981; VOL. 246; NO 1; PART. 1; PP. 74-85; BIBL. 11 REF.Article

THE CALIBRATION MAP OF THE HII REGION S237 IN HALPHA EMISSIONMIZUNO S; SAKKA K; SASAKI T et al.1981; ASTROPHYS. SPACE SCI.; ISSN 0004-640X; NLD; DA. 1981; VOL. 78; NO 1; PP. 235-242; BIBL. 10 REF.Article

SMALL-SCALE VELOCITY FIELDS AND MEAN LINE PROFILESDURRANT CJ.1980; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1980; VOL. 91; NO 1-2; PP. 251-253; BIBL. 4 REF.Article

EFFET DES DECALAGES SPECTRAUX DEVANT ET A COTE D'UNE MASSE SUR LE PROFIL DES RAIES SPECTRALES ISSUES DE CETTE MASSE OU DE MASSES LOCALISEES DERRIERE ELLEBORSENBERGER J; PECKER JC.1979; BULL. SOC. R. SCI. LIEGE; BEL; DA. 1979; VOL. 48; NO 5-8; PP. 204-211; ABS. ENG; BIBL. 1 REF.Article

ON THE USE OF LINE SHAPES IN THE ANALYSIS OF QSO ABSORPTION SPECTRA.WEISHEIT JC.1978; ASTROPHYS. J.; U.S.A.; DA. 1978; VOL. 219; NO 3 PART. 1; PP. 829-835; BIBL. 1/2 P.Article

DEMI-LARGEURS STANDARD DES RAIES DE LA BRANCHE R DE LA BANDE 2MU ₃ DE CH₄MALBROUCK R.1978; ACAD. R. BELG., BULL. CL. SCI.; BEL; DA. 1978; VOL. 64; NO 4; PP. 169-176; BIBL. 12 REF.Article