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

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

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

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

LE RAYONNEMENT DU NOYAU DE LA GALAXIE DE SEYFERT NGC 4151 DANS LES RAIES LAMBDA 4959 ET 5007 A (O III)PRONIK VI.1978; IZVEST. KRYM. ASTROFIZ. OBS.; S.S.S.R.; DA. 1978; VOL. 58; PP. 104-108; ABS. ANGL.; BIBL. 9 REF.Article

A NEW METHOD FOR DETERMINING DOPPLER WIDTHSSTEINITZ R; BAR V; WYCKOFF S et al.1975; ASTROPHYS. J.; USA; DA. 1975; VOL. 201; NO 3 PART. 1; PP. 729-734; BIBL. 22 REF.Article

CALCULS DE MONTE CARLO DE LA FORMATION DES RAIES DE RESONANCE DANS LES COUCHES PLANESVLASOV YU P; TITARCHUK LG.1982; PIS'MA V ASTRONOMICESKIJ ZURNAL; ISSN 507806; SUN; DA. 1982; VOL. 8; NO 9; PP. 566-572; ABS. ENG; BIBL. 9 REF.Article

A UNIFIED TREATMENT OF ESCAPE PROBABILITIES IN STATIC AND MOVING MEDIA. I: PLANE GEOMETRYHUMMER DG; RYBICKI GB.1982; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1982; VOL. 254; NO 2; PART. 1; PP. 767-779; BIBL. 12 REF.Article

FORMATION OF PERMITTED LINES IN THE SPECTRUM OF TYPE 1 SEYFERT GALAXIES AND QUASARS. II: FE II LINES AND THE LOW EXCITATION REGIONCOLLIN SOUFFRIN S; DUMONT S; HEIDMANN N et al.1980; ASTR. AND ASTROPHYS.; DEU; DA. 1980; VOL. 83; NO 1-2; PP. 190-198; BIBL. 37 REF.Article

LINE FORMATION IN RANDOM VELOCITY FIELDSGAIL HP; SEDLMAYR E; TRAVING G et al.1980; J. QUANT. SPECTROSC. RAD. TRANSFER; GBR; DA. 1980; VOL. 23; NO 3; PP. 267-284; BIBL. 16 REF.Article

STARK BROADENING TRENDS IN HOMOLOGOUS IONSMILLER MH; LESAGE A; PURIC J et al.1980; ASTROPHYS. J.; USA; DA. 1980; VOL. 239; NO 1; PART. 1; PP. 410-413; BIBL. 27 REF.Article

A COMPARISON OF THREE METHODS FOR COMPUTING LINE PROFILES IN SPHERICAL ENVELOPESBASTIAN U; BERTOUT C; STENHOLM L et al.1980; ASTR. AND ASTROPHYS.; DEU; DA. 1980; VOL. 86; NO 1-2; PP. 105-112; BIBL. 18 REF.Article