kw.\*:(%22SPECTRAL LINE WIDTH%22)
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A CRITERION FOR THE MEASUREMENT OF EQUIVALENT WIDTHSCRIVELLARI L; MARDIROSSIAN F; MOROSSI C et al.1979; ASTR. AND ASTROPHYS.; DEU; DA. 1979; VOL. 72; NO 1-2; PP. 256-260; BIBL. 4 REF.Article
DESIGNING A MICROSTRIPLINE.WAHI PK; RAMESH GARG.1977; J. INSTIT. ELECTRON. TELECOMMUNIC. ENGRS; INDIA; DA. 1977; VOL. 23; NO 7; PP. 445-447; BIBL. 10 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
SIMPLE LINEWIDTH-REDUCING MODIFICATION FOR A HANSCH DYE LASERGALLAGHER TF; KACHRU R; GOUNAND F et al.1982; APPL. OPT.; ISSN 0003-6935; USA; DA. 1982; VOL. 21; NO 3; PP. 363-364; BIBL. 1 REF.Article
MEASUREMENTS OF THE VELOCITY AND WIDTH OF THE H22.1 MICRON EMISSION LINE FROM THE ORION NEBULAOGDEN PM; ROESLER FL; REYNOLDS RJ et al.1978; ASTROPHYS. J.; USA; DA. 1978; VOL. 226; NO 2 PART. 2; PP. L91-L94; BIBL. 19 REF.Article
ON THE BALDWIN EFFECT IN OPTICALLY-SELECTED QUASARSKIANG T; CHENG FH; ZHOU YY et al.1983; MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY; ISSN 0035-8711; GBR; DA. 1983; VOL. 203; NO 2; PP. 25P-29P; BIBL. 11 REF.Article
LARGEURS EQUIVALENTES DES RAIES SOLAIRES DANS L'INTERVALLE SPECTRAL 8700-12000 ASITNIK GF.1979; SOOBSHCH. GOS. ASTR. INST. P.K. SHTERNBERGA; SUN; DA. 1979; NO 214-215; PP. 50-59; ABS. ENG; BIBL. 9 REF.Article
METHODES NUMERIQUES DE CORRECTION DES PROFILS DE RAIES SPECTRALES OBSERVES SUIVANT L'INFLUENCE DE L'INSTRUMENT.SATTAROV I.1978; ASTR. ZH.; SUN; DA. 1978; VOL. 55; NO 3; PP. 649-659; ABS. ENG; BIBL. 7 REF.Article
DIRECT OBSERVATION OF LORENTZIAN LINESHAPE OF SEMICONDUCTOR LASER AND LINEWIDTH REDUCTION WITH EXTERNAL GRATING FEEDBACKSAITO S; YAMAMOTO Y.1981; ELECTRON. LETT.; ISSN 0013-5194; GBR; DA. 1981; VOL. 17; NO 9; PP. 325-327; BIBL. 11 REF.Article
A POSSIBLE SOURCE OF SYSTEMATIC DISCREPANCIES IN THE EQUIVALENT WIDTH SCALES OF STELLAR ABSORPTION LINES.MITTON J.1976; ASTR. AND ASTROPHYS.; GERM.; DA. 1976; VOL. 50; NO 3; PP. 451-453; BIBL. 4 REF.Article
PLASMON LINEWIDTH AND FREQUENCY SHIFT IN DENSE MATTERITOH N; KOHYAMA Y; ICHMARU S et al.1982; PHYSICAL REVIEW LETTERS; ISSN 0031-9007; USA; DA. 1982; VOL. 49; NO 26; PP. 1932-1935; BIBL. 19 REF.Article
OBSERVATIONS SPECTRALES DE TROIS GALAXIES A EXCES UVKAZARYAN MA; TAMAZYAN VS.1982; PIS'MA ASTRON. Z.; ISSN 507806; SUN; DA. 1982; VOL. 8; NO 8; PP. 454-457; ABS. ENG; BIBL. 2 REF.Article
PROPERTIES OF THE SOLAR CHROMOSPHERE HALPHA SPICULES AS OBSERVED SPECTRALLYKULIDZANISHVILI VI; NIKOLSKY GM.1978; SOLAR PHYS.; NLD; DA. 1978; VOL. 59; NO 1; PP. 21-28; BIBL. 6 REF.Article
DETERMINATION DE LA LARGEUR DES PICS RADIOCRISTALLOGRAPHIQUES DANS LE CAS DE SUPERPOSITION MUTUELLEMUKHENBERG KM.1978; ZAVODSK. LAB.; SUN; DA. 1978; VOL. 44; NO 5; PP. 549-550; BIBL. 3 REF.Article
EMISSION LINES IN THE WINGS OF CA II H AND K. II. STELLAR OBSERVATIONS: DEPENDENCE OF LINE WIDTH ON LUMINOSITY AND RELATED TOPICS.STENCEL RE.1977; ASTROPHYS. J.; U.S.A.; DA. 1977; VOL. 215; NO 1 PART. 1; PP. 176-187; BIBL. 57 REF.Article
INFLUENCE DE LA MIGRATION D'ENERGIE OPTIQUE SUR LE CONTOUR DE L'ELARGISSEMENT NON HOMOGENE DANS LE SPECTRE DE LUMINESCENCEYAKOVLEV SV.1977; OPT. I SPEKTROSK.; S.S.S.R.; DA. 1977; VOL. 43; NO 2; PP. 258-260; BIBL. 7 REF.Article
INTERPRETATION DES RAIES D'ABSORPTION FAIBLES DANS LE SPECTRE DE VENUS)ANIKONOV AS.1977; ASTR. ZH.; S.S.S.R.; DA. 1977; VOL. 54; NO 1; PP. 169-177; ABS. ANGL.; BIBL. 15 REF.Article
LARGEURS EQUIVALENTES ET CATALOGUE DES RAIES SPECTRALES POUR LES COMPOSANTES PRIMAIRES ET SECONDAIRES DES BETA LYRAEDADAEV AN.1976; IZVEST. GLAVN. ASTR. OBS. PULKOVE; S.S.S.R.; DA. 1976; NO 194; PP. 18-35; ABS. ANGL.; BIBL. 14 REF.Article
K EMISSION LINE WIDTHS IN THE SUN AND THE STARS.BAPPU MKV; SRIVANASAN KR.1977; MONTH. NOT. R. ASTR. SOC.; G.B.; DA. 1977; VOL. 178; NO 2; PP. 279-287; BIBL. 12 REF.Article
LARGEURS EQUIVALENTES DE RAIES SPECTRALES DANS LES ETOILES BDIDELON P.1982; ASTRON. ASTROPHYS., SUPPL. SER.; ISSN 0365-0138; DEU; DA. 1982; VOL. 50; NO 2; PP. 199-207; ABS. ENG; BIBL. 32 REF.Article
MODELE DE LA CHROMOSPHERE AU-DESSUS D'UNE REGION ACTIVE SUIVANT LES RAIES LALPHA , LBETA DE L'HYDROGENE ET LES RAIES UVBARANOVSKIJ EH A; SEVERNYJ AB.1979; IZVEST. KRYM. ASTROFIZ. OBS.; SUN; DA. 1979; VOL. 60; PP. 99-107; ABS. ENG; BIBL. 13 REF.Article
LES RAIES DES TERRES RARES DANS LE SPECTRE DU SOLEIL CONSIDERE COMME UNE ETOILESTEPANYAN NN; SHCHERBAKOVA ZA.1978; IZVEST. KRYM. ASTROFIZ. OBS.; S.S.S.R.; DA. 1978; VOL. 58; PP. 3-7; ABS. ANGL.; BIBL. 14 REF.Article
THE INFLUENCE OF SPATIAL RESOLUTION ON THE CA+K LINE WIDTH AND SHIFT IN A QUIESCENT PROMINENCEENGUOLD O; WIEHR E; WITTMANN A et al.1980; ASTR. AND ASTROPHYS.; DEU; DA. 1980; VOL. 85; NO 3; PP. 326-328; BIBL. 8 REF.Article
NMR-LINIENVERSCHMAELERUNGSEXPERIMENTE MIT GROSSEM RESONANZOFFSET ZUR UNTERSUCHUNG VON FESTKOERPERN = EXPERIENCES DE RETRECISSEMENT DES RAIES RMN AVEC GRAND DECALAGE DE RESONANCE POUR L'ETUDE DES SOLIDESMUELLER R; SCHELER G.1979; ANN. PHYS.; DDR; DA. 1979; VOL. 36; NO 4; PP. 304-316; ABS. ENG; BIBL. 11 REF.Article
ELECTRONIC LINEWIDTH NARROWING METHOD FOR SINGLE AXIAL MODE OPERATION OF Q-SWITCHED ND:YAG LASERSPARK YK; BYER RL.1981; OPT. COMMUN.; ISSN 0030-4018; NLD; DA. 1981; VOL. 37; NO 6; PP. 411-416; BIBL. 17 REF.Article
