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ANGLE-AVERAGED REDISTRIBUTION FUNCTION IN THE LABORATORY FRAMESEITZ M; BASCHEK B; WEHRSE R et al.1982; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1982; VOL. 109; NO 1; PP. 10-16; BIBL. 23 REF.Article

COMMENTS ON THE REDISTRIBUTION FUNCTION OF JEFFERIES AND WHITE.KNEER F.1975; ASTROPHYS. J.; U.S.A.; DA. 1975; VOL. 200; NO 2 PART. 1; PP. 367-368; BIBL. 9 REF.Article

HYDROGEN LINE AND CONTINUUM EMISSION IN QUASARSKWAN J; KROLIK JH.1979; ASTROPHYS. J.; USA; DA. 1979; VOL. 233; NO 3 PART. 2; PP. L91-L95; BIBL. 40 REF.Article

BLANKETING EFFECT DU AUX MOLECULES TIOKIPPER TA.1979; PIS'MA ASTR. ZH.; SUN; DA. 1979; VOL. 5; NO 1; PP. 39-41; ABS. ENG; BIBL. 5 REF.Article

FORMATION DES RAIES SPECTRALES AVEC LOI GENERALE DE REDISTRIBUTIONNIKOGOSYAN AG; ARUTYUNYAN GA.1976; DOKL. AKAD. NAUK S.S.S.R.; S.S.S.R.; DA. 1976; VOL. 229; NO 3; PP. 583-586; BIBL. 8 REF.Article

INTERACTION BETWEEN EMISSION-LINE FILAMENTS AND HIGHLY ENERGETIC EXPLOSIONS IN QSOSMARSCHER AP.1978; ASTROPHYS. J.; USA; DA. 1978; VOL. 225; NO 3 PART. 1; PP. 725-731; BIBL. 32 REF.Article

THE EFFECTIVE OPTICAL DEPTH FOR THE FORMATION OF ABSORPTION LINESMAKITA M.1977; SOLAR PHYS.; NLD; DA. 1977; VOL. 51; NO 1; PP. 43-49; BIBL. 10 REF.Article

THE MEAN PHOTON PATH LENGTH IN EXTREMELY OPAQUE MEDIAADAMS TF.1975; ASTROPHYS. J.; USA; DA. 1975; VOL. 201; NO 2 PART. 1; PP. 350-351; BIBL. 7 REF.Article

EFFECTIVE DEPTH OF SPECTRAL LINE FORMATION IN PLANETARY ATMOSPHERESLESTRADE JP; CHAMBERLAIN JW.1980; ICARUS; ISSN 0019-1035; USA; DA. 1980; VOL. 44; NO 3; PP. 813-815; BIBL. 8 REF.Article

EXCITATION OF MGII AND FEII LINES IN QUASARS AND SEYFERT GALAXIESNETZER H.1980; ASTROPHYS. J.; USA; DA. 1980; VOL. 236; NO 2 PART. 1; PP. 406-418; BIBL. 62 REF.Article

LINE FORMATION IN TURBULENT MEDIA WITH FINITE CORRELATION LENGTHSTAHLBERG J.1979; ASTR. NACHR.; DDR; DA. 1979; VOL. 300; NO 5; PP. 261-267; ABS. GER; BIBL. 9 REF.Article

RESONANCE LINE POLARIZATION: THE LINE CORE.DUMONT S; OMONT A; PECKER JC et al.1977; ASTR. AND ASTROPHYS.; GERM.; DA. 1977; VOL. 54; NO 3; PP. 675-681; BIBL. 13 REF.Article

ETUDE DE LA FORMATION DES RAIES MILLIMETRIQUES DE MOLECULES DANS LES NUAGES INTERSTELLAIRES.LUCAS R.1976; AO-CNRS-12592; FR.; DA. 1976; PP. 1-82; BIBL. 2 P.; (THESE DOCT. ETAT SCI. PHYS.; PIERRE ET MARIE CURIE PARIS 6)Thesis

LINE FORMATION IN EXPANDING ATMOSPHERES: ON THE VALIDITY OF THE SOBOLEV APPROXIMATIONHAMANN WR.1981; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1981; VOL. 93; NO 1-2; PP. 353-361; BIBL. 11 REF.Article

MECHANICAL FLUX IN THE SOLAR CHROMOSPHERE. II: DETERMINATION OF THE MECHANICAL FLUXSCHMIEDER B; MEIN N.1980; ASTR. AND ASTROPHYS.; DEU; DA. 1980; VOL. 84; NO 1-2; PP. 99-105; BIBL. 32 REF.Article

LINE FORMATION IN SPHERICAL MEDIA WITH PARTITAL FREQUENCY REDISTRIBUTION. II: EXPANDING MEDIA WITH REDISTRIBUTION FUNCTION R1PERAIAH A.1979; ASTROPHYS. SPACE SCI.; NLD; DA. 1979; VOL. 63; NO 2; PP. 267-277; BIBL. 17 REF.Article

L'EMISSION DU FLUX DE PROTONS SUPRATHERMIQUES TRAVERSANT UN GAZ NEUTRE ET LE MECANISME DE FORMATION DES RAIES LARGES DANS LES NOYAUX DES GALAXIES DE SEYFERTPRONIK VI.1977; IZVEST. KRYM. ASTROFIZ. OBS.; S.S.S.R.; DA. 1977; VOL. 56; PP. 59-67; BIBL. 4 REF.Article

THE SCATTERING EFFECTS OF THE REDISTRIBUTION FUNCTION RIII(X',N';X,N) ON SPECTRAL LINE FORMATION.VARDAVAS IM.1976; J. QUANT. SPECTROSC. RAD. TRANSFER; G.B.; DA. 1976; VOL. 16; NO 8; PP. 715-719; BIBL. 7 REF.Article

S 106: AN H II-REGION DRIVEN BY A STELLAR WIND.HIPPELEIN H; MUENCH G.1981; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1981; VOL. 99; NO 2; PP. 248-254; BIBL. 29 REF.Article

PROFONDEUR OPTIQUE DE FORMATION DES RAIES DE FRAUNHOFER FAIBLESSARYCHEV AP.1981; ASTR. ZH.; SUN; DA. 1981; VOL. 58; NO 2; PP. 403-407; ABS. ENG; BIBL. 12 REF.Article

SODIUM D-LINE EMISSION FROM IO: A SECOND YEAR OF SYNOPTIC OBSERVATION FROM TABLE MOUNTAIN OBSERVATORY.BERGSTRALH JT; YOUNG JW; MATSON DL et al.1977; ASTROPHYS. J.; U.S.A.; DA. 1977; VOL. 211; NO 1 PART. 2; PP. L51-L55; BIBL. 9 REF.Article

LINE FORMATION IN EXPANDING ATMOSPHERES.HUMMER DG.1976; INTERNATION. ASTR. UN., SYMP.; NETHERL.; DA. 1976; NO 70; PP. 281-312; BIBL. 2 P.; (BE AND SHELL STARS. MERRILL-MCLAUGHLIN MEM. SYMP.; BASS RIVER, MASS.; 1975)Conference Paper

REFINED MONTE CARLO METHOD FOR SIMULATING ANGLE-DEPENDENT PARTIAL FREQUENCY REDISTRIBUTIONSJONG SEN LEE.1982; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1982; VOL. 255; NO 1; PART. 1; PP. 303-306; BIBL. 6 REF.Article

THE IMPLICATIONS OF HYDROGEN EMISSION LINE RATIOS IN QUASI-STELLAR OBJECTSCANFIELD RC; PUETTER RC.1980; ASTROPHYS. J.; USA; DA. 1980; VOL. 236; NO 1 PART. 2; PP. 7-11; BIBL. 24 REF.Article

ON THE WIDTH OF SPECTRAL LINESBERTOUT C.1978; ASTR. AND ASTROPHYS.; DEU; DA. 1978; VOL. 70; NO 3; PP. 447-450; BIBL. 9 REF.Article

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