POLARIZATION IN THE EMISSION LINES OF BE STARS.COYNE GV.1976; ASTR. AND ASTROPHYS.; GERM.; DA. 1976; VOL. 49; NO 1; PP. 89-96; BIBL. 28 REF.Article

THE LOW EXCITATION SPECTRUM OF THE PECULIAR STAR WITH INFRARED EXCESS RX PUPPIS IN 1972 AND 1975.SWINGS JP; KLUTZ M.1976; ASTR. AND ASTROPHYS.; GERM.; DA. 1976; VOL. 46; NO 2; PP. 303-311; BIBL. 27 REF.Article

EMISSION-LINE SPECTRA OF INDIVIDUAL CONDENSATIONS OF HERBIG-HARO OBJECTS.BOHM KH; SIEGMUND WA; SCHWARTZ RD et al.1976; ASTROPHYS. J.; U.S.A.; DA. 1976; VOL. 203; NO 2 PART. 1; PP. 399-409; BIBL. 30 REF.Article

OBSERVATIONS OF WOLF-RAYET STARS IN THE EMISSION-LINE GALAXY TOLOLO 3KUNTH D; SARGENT WLW.1981; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1981; VOL. 101; NO 2; PP. L5-L8; BIBL. 24 REF.Article

KI 7699 A EMISSION FROM THE BETELGEUSE SHELL.BERNAT AP; LAMBERT DL.1976; ASTROPHYS. J.; U.S.A.; DA. 1976; VOL. 210; NO 2 PART. 1; PP. 395-401; BIBL. 17 REF.Article

FE I FLUORESCENCE IN T TAURI STARS.WILLSON LA.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 191; NO 1 PART. 1; PP. 143-155; BIBL. 21 REF.Article

THE BEHAVIOR OF THE MG II DOUBLET EMISSIONS NEAR 2800 A OBSERVED IN LATE-TYPE GIANTS.KONDO Y; MORGAN TH; MODISETTE JL et al.1976; ASTROPHYS. J.; U.S.A.; DA. 1976; VOL. 207; NO 1 PART. 1; PP. 167-173Article

THE COMPLEX STRUCTURE OF THE CAII (H AND K) LINES IN THE SPECTRUM OF THE AOEP STAR WITH INFRARED EXCESS HD 190073. II. INTERPRETATION: THE SELECTIVE EFFECT OF RADIATIVE FORCES.SURDEJ J; SWINGS JP.1976; ASTR. AND ASTROPHYS.; GERM.; DA. 1976; VOL. 47; NO 1; PP. 121-127; BIBL. 15 REF.Article

JETS FROM PRE-MAIN-SEQUENCE STARS: AS 353A AND ITS ASSOCIATED HERBIG-HARO OBJECTSMUNDT R; STOCKE J; STOCKMAN HS et al.1983; ASTROPHYSICAL JOURNAL; ISSN 0004-637X; USA; DA. 1983; VOL. 265; NO 2; PART. 2; PP. L71-L75; H.T. 2; BIBL. 18 REF.Article

OUTER ATMOSPHERES OF COOL STARS. IX: A SURVEY OF ULTRAVIOLET EMISSION FROM F-K DWARFS AND GIANTS WITH IUEAYRES TR; MARSTAD NC; LINSKY JL et al.1981; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1981; VOL. 247; NO 2; PART. 1; PP. 545-559; BIBL. 90 REF.Article

STELLAR MODEL CHROMOSPHERES. XII. HIGH-RESOLUTION, ABSOLUTE FLUX PROFILES OF THE CA_II H AND K LINES IN DME AND NON-DME STARSGIAMPAPA MS; CRAM LE.1981; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1981; VOL. 246; NO 2; PART. 1; PP. 502-514; BIBL. 37 REF.Article

A RADIAL VELOCITY STUDY OF EMISSION IN STEPANYAN'S STARYOUNG P; SCHNEIDER DP; SHECTMAN SA et al.1981; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1981; VOL. 244; NO 1; PART. 1; PP. 259-268; BIBL. 11 REF.Article

COLLAPSING MOLECULAR CLOUDS.LOREN RB; PETERS WL; VANDEN BOOT PA et al.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 194; NO 2 PART. 2; PP. 103-107; BIBL. 14 REF.Article

SEPT NOUVELLES ETOILES B AYANT LA RAIE HALPHA EN EMISSION.DOAZAN V; BOURDONNEAU B; LETOURNEUR N et al.1977; ASTR. AND ASTROPHYS.; GERM.; DA. 1977; VOL. 56; NO 3; PP. 481-482; ABS. ANGL.; BIBL. 12 REF.Article

THE FEII AND (FEII) EMISSION LINE STAR R50 IN THE SMALL MAGELLANIC CLOUD.MAURICE E.1976; ASTR. AND ASTROPHYS.; GERM.; DA. 1976; VOL. 50; NO 3; PP. 463-466; BIBL. 13 REF.Article

ULTRAVIOLET SI IV/CIV RATIOS FOR BE STARS.HENIZE KG; WRAY JD; PARSONS SB et al.1976; INTERNATION. ASTR. UN., SYMP.; NETHERL.; DA. 1976; NO 70; PP. 191-195; BIBL. 6 REF.; (BE AND SHELL STARS. MERRILL-MCLAUGHLIN MEM. SYMP.; BASS RIVER, MASS.; 1975)Conference Paper

NEW BRIGHT HYDROGEN-EMISSION STARS.IRVINE NJ.1975; ASTROPHYS. J.; U.S.A.; DA. 1975; VOL. 196; NO 3 PART. 1; PP. 773-775; BIBL. 24 REF.Article

SS 433: HOW THE MOVING LINES MOVEGRANDI SA; STONE RPS.1982; PUBL. ASTRON. SOC. PAC.; ISSN 0004-6280; USA; DA. 1982; VOL. 94; NO 557; PP. 80-86; BIBL. 14 REF.Article

A SPECTROSCOPIC SURVEY OF EMISSION-LINE OBJECTS IN TWO FIELDSKUNTH D; SARGENT WLW; KOWAL C et al.1981; ASTRON. ASTROPHYS., SUPPL. SER.; ISSN 0365-0138; DEU; DA. 1981; VOL. 44; NO 2; PP. 229-239; BIBL. 10 REF.Article

SUSPECTED VARIABILITY AND LINE EMISSION IN EARLY-TYPE STARSIRVINE NJ; IRVINE CE.1979; PUBL. ASTR. SOC. PACIF.; USA; DA. 1979; VOL. 91; NO 539; PP. 105-106; BIBL. 10 REF.Article

A FINDING LIST OF HALPHA -EMISSION OBJECTS IN THE COALSACK DIRECTION.GOMEZ T; MENDOZA VEE.1976; REV. MEX. ASTR. ASTROFIS.; MEXICO; DA. 1976; VOL. 1; NO 4; PP. 381-384; H.T. 56; ABS. ESP.; BIBL. 3 REF.Article

ALTERNATIVE EXPLANATION FOR THE SPECTRAL LINES OBSERVED IN QUASARS.VARSHNI YP.1975; ASTROPHYS. SPACE SCI.; NETHERL.; DA. 1975; VOL. 37; NO 1; PP. L1-L6; BIBL. DISSEM.Article

OPTICAL LINE EMISSION FROM IO.BROWN RA.1974; INTERNATION. ASTR. UN., SYMP.; NETHERL.; DA. 1974; NO 65; PP. 527-531; BIBL. 4 REF.; (EXPLOR. PLANET. SYST. COPERNICUS SYMP. IV; TORUN, POL.; 1973)Conference Paper

LABORATORY PRODUCED VISIBLE SPECTRAL EMISSION FEATURES CORRELATE WITH THOSE OF THE RED RECTANGLEWDOWIAK TJ.1981; NATURE (LOND.); GBR; DA. 1981; VOL. 293; NO 5835; PP. 724-725; BIBL. 7 REF.Article

EMISSION OBJECT IN ORION.GEIBELMAN WA.1976; PUBL. ASTR. SOC. PACIF.; U.S.A.; DA. 1976; VOL. 88; NO 525; PP. 677-679; BIBL. 6 REF.Article