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NUCLEAR ASTROPHYSICS. THE ORIGIN OF HEAVY ELEMENTS.SCHRAMM DN.1976; NUKLEOMIKA; POLSKA; DA. 1976; VOL. 21; NO 6; PP. 727-751; ABS. POL. RUSSE; BIBL. 2 P.Article

ENRICHMENT OF HEAVY ELEMENTS IN THE GALAXY: A SIMPLE FORMULA.DORNSCHNER J; JUERTLER J.1976; ASTR. NACHR.; DTSCH.; DA. 1976; VOL. 297; NO 1; PP. 25-27; ABS. ALLEM.; BIBL. 3 REF.Article

SEGREGATION OF THE HEAVY ELEMENTS IN THE SOLAR SYSTEM.WILLIAMS IP; HANDBURY MJ.1974; ASTROPHYS. SPACE SCI.; NETHERL.; DA. 1974; VOL. 30; NO 1; PP. 215-233; BIBL. 14 REF.Article

SOME RECENT RESULTS FROM GALACTIC AND STELLAR EVOLUTION THEORY.TALBOT RJ JR; ARNETT WD.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 109; NO 3 PART. 1; PP. 605-608; BIBL. 16 REF.Article

ARE STELLAR SURFACE HEAVY-ELEMENT ABUNDANCES SYSTEMATICALLY ENHANCED.JOSS PC.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 191; NO 3 PART. 1; PP. 771-774; BIBL. 43 REF.Article

CHEMICAL EVOLUTION OF GALAXIES. II: VARIATION OF THE HEAVY ELEMENT YIELD WITH ZPEIMBERT M; SERRANO A.1982; MON. NOT. R. ASTRON. SOC.; ISSN 0035-8711; GBR; DA. 1982; VOL. 198; NO 2; PP. 563-572; BIBL. 61 REF.Article

RADIOISOTOPES APPLIED TO ENVIRONMENTAL TOXICITY RESEARCH WITH MICROBESKOKKE R.1972; IN: RADIOTRACER STUD. CHEM. RESIDUES FOOD AGRIC. PROC. COMBINED PANEL RES. COORD. MEET. VIENNA, 1971; VIENNA; I.A.E.A.; DA. 1972; PP. 15-23; BIBL. 14Conference Proceedings

CORRELATION AGE-METALLICITE DETERMINEE SPECTROSCOPIQUEMENT POUR DES ETOILES DE LA POPULATION DU DISQUEVERESHCHAGIN SV.1981; ASTR. SOVET AKAD. NAUK S.S.S.R., NAUCH. INFORM.; SUN; DA. 1981; VOL. 47; PP. 51-58; ABS. ENG; BIBL. 18 REF.Article

A SEMIEMPIRICAL MODEL FOR HEAVY ELEMENT DEPLETION IN THE INTERSTELLAR MEDIUMTRIVEDI BMP; LARIMER JW.1981; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1981; VOL. 248; NO 2; PART. 1; PP. 563-568; BIBL. 31 REF.Article

HEAVY ELEMENT ENRICHMENT OF THE INTERGALACTIC MEDIUMOBER WW.1980; COSMOLOGIE PHYSIQUE. ECOLE D'ETE DE PHYSIQUE THEORIQUE. SESSION. 32/1979/LES HOUCHES; NLD/USA/GBR; AMSTERDAM: NORTH-HOLLAND/NEW YORK: NORTH-HOLLAND/OXFORD: NORTH-HOLLAND; DA. 1980; PP. 661-665; BIBL. 14 REF.Conference Paper

ON THE ABUNDANCE OF HEAVY ELEMENTS IN THE GALACTIC CENTRE.AITKEN DK; GRIFFITHS J; JONES B et al.1976; MONTH. NOT. R. ASTR. SOC.; G.B.; DA. 1976; VOL. 176; NO 3; PP. 73P-77P; BIBL. 13 REF.Article

ELECTRONIC SYSTEM FOR HIGH SENSITIVITY AND HIGH STABILITY MASS SPECTROMETRY. II. ELECTRONIC SET-UP FOR AN "ON-LINE" MASS SPECTROMETERGOBY G; LONG DEN NGUYEN.1973; INTERNATION. J. MASS SPECTROM. ION PHYS.; NETHERL.; DA. 1973; VOL. 11; NO 3; PP. 215-221; BIBL. 2 REF.Serial Issue

A PLEA FOR REEXAMINING HEAVY ELEMENT OPACITIES IN STARSSIMON NR.1982; ASTROPHYSICAL JOURNAL; ISSN 0004-637X; USA; DA. 1982; VOL. 260; NO 2; PART. 2; PP. 87-90; BIBL. 28 REF.Article

R-PROCESS NUCLEOSYNTHESIS: A DYNAMICAL MODEL.HILLEBRANDT W; TAKAHASHI K; KODAMA T et al.1976; ASTR. AND ASTROPHYS.; GERM.; DA. 1976; VOL. 52; NO 1; PP. 63-68; BIBL. 14 REF.Article

DO COMETS PLAY A ROLE IN GALACTIC CHEMISTRY AND GAMMA -RAY BURSTS.WHIPPLE FL.1975; ASTR. J.; U.S.A.; DA. 1975; VOL. 80; NO 7; PP. 525-531; BIBL. 26 REF.Article

STUDIES OF HEAVY-ELEMENT SYNTHESIS IN THE GALAXY. I. SEPARATION OF R-AND S-PROCESS ABUNDANCESBUTCHER HR.sdASTROPHYS. J.; U.S.A.; DA. 197; VOL. 176; NO 3, PART 1; PP. 711-722; BIBL. 39REF.Serial Issue

THE CHEMICAL COMPOSITION, STRUCTURE, AND DYNAMICS OF GLOBULAR CLUSTERSFREEMAN KC; NORRIS J.1981; ANNU. REV. ASTRON. ASTROPHYS.; ISSN 0066-4146; USA; DA. 1981; VOL. 19; PP. 319-356; BIBL. 2 P.Article

DEPLETION OF HEAVY ELEMENTS TOWARD THE RHO OPHIUCHI DUST CLOUD.CRUTCHER RM.1976; ASTROPHYS. J.; U.S.A.; DA. 1976; VOL. 208; NO 2 PART. 1; PP. 382-389; BIBL. 25 REF.Article

SENSITIVITY OF THE STAR FORMATION RATE TO THE INTERSTELLAR GAS ABUNDANCE OF HEAVY ELEMENTS.TALBOT RJ JR.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 189; NO 2 PART. 1; PP. 209-215; BIBL. 37 REF.Article

THE HEAVY ELEMENT YIELDS OF NEUTRON CAPTURE NUCLEOSYNTHESISCAMERON AGW.1982; ASTROPHYS. SPACE SCI.; ISSN 0004-640X; NLD; DA. 1982; VOL. 82; NO 1; PP. 123-131; BIBL. 8 REF.Article

A PREGALACTIC POPULATION III: PRIMORDIAL HELIUM AND HEAVY ELEMENTS AND THE MICROWAVE BACKGROUNDTARBET PW; ROWAN ROBINSON M.1982; NATURE (LONDON); ISSN 0028-0836; GBR; DA. 1982; VOL. 298; NO 5876; PP. 711-715; BIBL. 50 REF.Article

PROPERTIES OF A SAMPLE OF IRREGULAR GALAXIES.ALLOIN D; BERGERON J; PELAT D et al.1978; ASTR. AND ASTROPHYS.; DEU; DA. 1978; VOL. 70; NO 1-2; PP. 141-149; BIBL. 45 REF.Article

SOLAR-SYSTEM ABUNDANCES OF NUCLIDES AND NUCLEAR STRUCTUREANAGNOSTATOS GS.1977; ASTROPHYS. SPACE SCI.; NLD; DA. 1977; VOL. 50; NO 2; PP. 445-450; BIBL. 26 REF.Article

SPUTTERING IN INTERSTELLAR SHOCKS: A MODEL FOR HEAVY ELEMENT DEPLETION.BARLOW MJ; SILK J.1977; ASTROPHYS. J.; U.S.A.; DA. 1977; VOL. 211; NO 2 PART. 2; PP. L83-L87; BIBL. 23 REF.Article

OBSERVATIONS OF HEAVY-ELEMENT RECOMBINATION LINES IN THE RHO OPHIUCHI DARK CLOUD AT 13 CENTIMETERS WAVELENGTH.KNAPP GR; KUIPER TBH; BROWN RL et al.1976; ASTROPHYS. J.; U.S.A.; DA. 1976; VOL. 206; NO 1 PART. 1; PP. 109-113; BIBL. 21 REF.Article

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