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HIGH REDSHIFT 21-CM LINES.ROBERTS MS.1977; IN: DECALAGES VERS ROUGE EXPANS. UNIVERS. UNION ASTRON. INT. COLLOQ. 37. EVOL. GALAXIES IMPLICATIONS COSMOL. CNRS. COLL. INT. 263; PARIS; 1976; PARIS; CNRS; DA. 1977; PP. 501-509; ABS. FR.; BIBL. 10 REF.Conference Paper

OBSERVATIONAL CONSTRAINTS ON GALAXY-IGM INTERACTIONS IN THE VIRGO CLUSTERSTAUFFER JR.1983; ASTROPHYSICAL JOURNAL; ISSN 0004-637X; USA; DA. 1983; VOL. 264; NO 1; PART. 1; PP. 14-23; BIBL. 32 REF.Article

DOUBLE GALAXY INVESTIGATIONS. II: THE REDSHIFT PERIODICITY IN OPTICALLY OBSERVED PAIRSTIFFT WG.1982; ASTROPHYSICAL JOURNAL; ISSN 0004-637X; USA; DA. 1982; VOL. 262; NO 1; PART. 1; PP. 44-47; BIBL. 5 REF.Article

21-CM LINE PROFILES OF 40 SA SPIRAL GALAXIESBOTTINELLI L; GOUGUENHEIM L; PATUREL G et al.1980; ASTR. AND ASTROPHYS., SUPPL. SER.; DEU; DA. 1980; VOL. 40; NO 3; PP. 355-362Article

DISTANCE ESTIMATE FOR THE GALACTIC SUPERNOVA REMNANT G74.9+1.2 USING HI ABSORPTION-LINE MEASUREMENTS.SATO F.1977; PUBL. ASTR. SOC. JAP.; JAP.; DA. 1977; VOL. 29; NO 3; PP. 615-618; BIBL. 12 REF.Article

ETUDE DE LA CONSTANTE DE HUBBLE A PARTIR D'OBSERVATIONS DE GALAXIES EN RAIE 21 CM.DURAND N.1975; ; S.L.; DA. 1975; PP. 1-32; H.T. 50; BIBL. 2 P. 1/2; (THESE DOCT. UNIV., MENTION SCI.; PARIS VII)Thesis

A HIGH RESOLUTION HI SURVEY OF M31BRINKS E.1982; SYMPOSIUM - INTERNATIONAL ASTRONOMICAL UNION; ISSN 0074-1809; NLD; DA. 1982; NO 100; PP. 23-26; BIBL. 3 REF.Conference Paper

THE KINEMATICS OF THE LENTICULAR GALAXIES NGC 1291 AND NGC 1326 FROM 21 CM LINE OBSERVATIONSMEBOLD U; GOSS WM; VAN WOERDEN H et al.1979; ASTR. AND ASTROPHYS.; DEU; DA. 1979; VOL. 74; NO 1; PP. 100-107; BIBL. 29 REF.Article

ILLUSIONARY WARPS IN HI DISKS OF NEARLY EDGE-ON SPIRAL GALAXIES.BYRD GG.1978; ASTROPHYS. J.; U.S.A.; DA. 1978; VOL. 222; NO 3 PART. 1; PP. 815-820 (5P.); BIBL. 20 REF.Article

DETERMINATION DES PARAMETRES DE LA STRUCTURE SPIRALE DE LA GALAXIE A PARTIR DE LA RAIE A 21 CM DE L'HYDROGENE NEUTRE. I. THEORIE LINEAIRE. REGION NON RESONANTEBERMAN VG; MISHUROV YU N.1978; ASTROFIZIKA; SUN; DA. 1978; VOL. 14; NO 4; PP. 637-644; ABS. ENG; BIBL. 10 REF.Article

HI PROFILE DISTANCES AND THE HUBBLE CONSTANT.FISHER JR; TULLY RB.1977; COMMENTS ON ASTROPHYS.; G.B.; DA. 1977; VOL. 7; NO 3; PP. 85-93; BIBL. 17 REF.Article

CONTOUR MAPS OF THE LATITUDE DISTRIBUTION OF LOW-VELOCITY NEUTRAL HYDROGEN.SCHOBER J.1976; ASTR. AND ASTROPHYS., SUPPL. SER.; GERM.; DA. 1976; VOL. 25; NO 3; PP. 507-518; BIBL. 5 REF.Article

GALAXIEN IM LICHTE DER 21-CM-LINIE = LES GALAXIES A LA LUMIERE DE LA RAIE A 21 CMMEBOLD U; REIF K.1981; MITT. ASTRON. GES.; ISSN 0374-1958; DEU; DA. 1981; NO 51; PP. 143-158; ABS. ENG; BIBL. 36 REF.Article

STUDY OF ONE 21-CM COMPONENT FROM LOCAL INTERSTELLAR MATTER IN THE SOUTHERN SKYMORRAS R.1979; ASTROPHYS. LETTERS; USA; DA. 1979; VOL. 20; NO 2; PP. 45-48; BIBL. 14 REF.Article

-CM OBSERVATIONS OF REDSHIFTS AND THEIR IMPLICATIONS FOR THE DISTANCE SCALE.TULLY RB; FISHER JR.1977; IN: DECALAGES VERS ROUGE EXPANS. UNIVERS. UNION ASTRON. INT. COLLOQ. 37. EVOL. GALAXIES IMPLICATIONS COSMOL. CNRS. COLL. INT. 263; PARIS; 1976; PARIS; CNRS; DA. 1977; PP. 95-117; ABS. FR.; BIBL. 1 P.Conference Paper

FURTHER 21 CM SURVEY OBSERVATIONS IN THE SOUTHERN MILKY WAY.KERR FJ; BALL DL; HARTEN RH et al.1976; ASTR. AND ASTROPHYS., SUPPL. SER.; GERM.; DA. 1976; VOL. 25; NO 3; PP. 391-432; BIBL. 6 REF.Article

THE 21-CM ABSORPTION LINE IN NGC 1275.EKERS RD; VAN DER HULST JM; MILEY GK et al.1976; NATURE; G.B.; DA. 1976; VOL. 262; NO 5567; PP. 369-370; BIBL. 8 REF.Article

A 21 CM LONGITUDE VELOCITY DIAGRAM FOR THE GALACTIC EQUATOR, L=236O-340O.BALL DL; GRAYZEK EJ; HARTEN RH et al.1976; ASTR. AND ASTROPHYS., SUPPL. SER.; GERM.; DA. 1976; VOL. 25; NO 3; PP. 449-452Article

EFFECTIVE HI DIAMETERS OF GALAXIESFOUQUE P.1983; ASTRONOMY AND ASTROPHYSICS; ISSN 0004-6361; DEU; DA. 1983; VOL. 122; NO 1-2; PP. 273-281; BIBL. 24 REF.Article

EXTENDED ROTATION CURVES OF HIGH-LUMINOSITY SPIRAL GALAXIES. V: NGC 1961, THE MOST MASSIVE SPIRAL KNOWNRUBIN VC; FORD WK JR; ROBERTS MS et al.1979; ASTROPHYS. J.; USA; DA. 1979; VOL. 230; NO 1 PART. 1; PP. 35-39; BIBL. 12 REF.Article

A STATISTICAL STUDY OF LOCAL INTERSTELLAR MATTER BASED ON THE NANCAY 21-CM ABSORPTION SURVEYCROVISIER J; KAZES I.1979; INTERNATION. ASTR. UN., SYMP.; NLD; DA. 1979; NO 84; PP. 253-256; BIBL. 10 REF.Conference Paper

NEUTRAL HYDROGEN IN THE CARTWHEEL.MEBOLD U; GOSS WM; FOSBURY RAE et al.1977; MONTH. NOT. R. ASTR. SOC.; G.B.; DA. 1977; VOL. 180; NO 1; PP. 11P-13P; BIBL. 6 REF.Article

THE DISTANCE TO LOW-LATITUDE NEGATIVE-VELOCITY CLOUDS IN THE GALACTIC ANTICENTER.DENOYER LK; BUTTON L; CHAFFIN D et al.1977; ASTROPHYS. J.; U.S.A.; DA. 1977; VOL. 213; NO 2 PART. 1; PP. 379-385; BIBL. 40 REF.Article

THE H0 VALUE FROM LUMINOSITY CLASSES AND 21-CM LINE OBSERVATIONS OF GALAXIES.BOTTINELLI L; GOUGUENHEIM L.1977; IN: DECALAGES VERS ROUGE EXPANS. UNIVERS. UNION ASTRON. INT. COLLOQ. 37. EVOL. GALAXIES IMPLICATIONS COSMOL. CNRS. COLL. INT. 263; PARIS; 1976; PARIS; CNRS; DA. 1977; PP. 481-486; ABS. FR.; BIBL. 6 REF.Conference Paper

HIGH RESOLUTION HI OBSERVATIONS OF MESSIER 31BAJAJA E; SHANE WW.1982; ASTRON. ASTROPHYS., SUPPL. SER.; ISSN 0365-0138; DEU; DA. 1982; VOL. 49; NO 4; PP. 745-774; BIBL. 20 REF.Article

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