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ON THE SYNTHESIS OF NEUTRON-RICH IRON-PEAK NUCLEITRURAN JW.1972; ASTROPHYS. J.,; U.S.A.; DA. 1972; VOL. 177; NO 2; PP. 453-458; BIBL. 32REF.Serial Issue

BETA DECAY RATES FOR S-PROCESS STUDIESCOSNER K; TRURAN JW.1981; ASTROPHYS. SPACE SCI.; ISSN 0004-640X; NLD; DA. 1981; VOL. 78; NO 1; PP. 85-94; BIBL. 19 REF.Article

POSSIBLE TRANSFER OF LUNAR MATTER TO EARTH DUE TO A NEARBY SUPERNOVARUDERMAN M; TRURAN JW.1980; NATURE; GBR; DA. 1980; VOL. 284; NO 5754; PP. 328-329; BIBL. 14 REF.Article

DIFFUSION AND HYDROGEN SHELL BURNING ON SLOWLY ACCRETING WHITE DWARFSFUJIMOTO MY; TRURAN JW.1982; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1982; VOL. 257; NO 1; PART. 1; PP. 303-311; BIBL. 16 REF.Article

AN X-RAY MODEL FOR THE NEBULA OF NOVA DQ HERCULIS 1934FERLAND GJ; TRURAN JW.1981; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1981; VOL. 244; NO 3; PART. 1; PP. 1022-1032; BIBL. 54 REF.Article

THE SUPERNOVA TRIGGER FOR FORMATION OF THE SOLAR SYSTEM.CAMERON AGW; TRURAN JW.1977; ICARUS; U.S.A.; DA. 1977; VOL. 30; NO 3; PP. 447-461; BIBL. 1 P.Article

THE EVOLUTION OF MASSIVE STARS. II: THE INFLUENCE OF INITIAL COMPOSITION AND MASS LOSSBRUNISH WM; TRURAN JW.1982; ASTROPHYS. J., SUPPL. SER.; ISSN 0067-0049; USA; DA. 1982; VOL. 49; NO 3; PP. 447-468; BIBL. 26 REF.Article

ON THE CARBON COMPOSITION OF THE EJECTA OF DQ HERCULISFERLAND GJ; TRURAN JW.1980; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1980; VOL. 240; NO 2; PART. 1; PP. 608-611; BIBL. 23 REF.Article

26AL PRODUCTION IN EXPLOSIVE CARBON BURNING.TRURAN JW; CAMERON AGW.1978; ASTROPHYS. J.; U.S.A.; DA. 1978; VOL. 219; NO 1 PART. 1; PP. 226-229; BIBL. 18 REF.Article

THE P-PROCESS IN EXPLOSIVE NUCLEOSYNTHESISTRURAN JW; CAMERON AGW.1972; ASTROPHYS. J.; U.S.A.; DA. 1972; VOL. 171; NO 1, PART. 1; PP. 89-92; BIBL. 19REF.Serial Issue

ON THE SURFACE COMPOSITION OF THERMALLY PULSING STARS OF HIGH LUMINOSITY AND ON THE CONTRIBUTION OF SUCH STARS TO THE ELEMENT ENRICHMENT OF THE INTERSTELLAR MEDIUM.IBEN I JR; TRURAN JW.1978; ASTROPHYS. J.; USA; DA. 1978; VOL. 220; NO 3 PART. 1; PP. 980-995; BIBL. 72 REF.Article

ON S-PROCESS NUCLEOSYNTHESIS IN THERMALLY PULSING STARS.TRURAN JW; IBEN I JR.1977; ASTROPHYS. J.; U.S.A.; DA. 1977; VOL. 216; NO 3 PART. 1; PP. 797-810; BIBL. 56 REF.Article

CNO ABUNDANCES AND HYDRODYNAMIC STUDIES OF THE NOVA OUTBURST. V. 100 M MODELS WITH SMALL MASS ENVELOPESSTARRFIELD S; TRURAN JW; SPARKS WM et al.1978; ASTROPHYS. J.; USA; DA. 1978; VOL. 226; NO 1 PART. 1; PP. 186-202; BIBL. 67 REF.Article

A HYDRODYNAMIC STUDY OF A SLOW NOVA OUTBURST.SPARKS WM; STARRFIELD S; TRURAN JW et al.1978; ASTROPHYS. J.; USA; DA. 1978; VOL. 220; NO 3 PART. 1; PP. 1063-1075; BIBL. 38 REF.Article

CNO ABUNDANCES AND HYDRODYNAMIC MODELS OF THE NOVA OUTBURST. II. 1.00 MO MODELS WITH ENHANCED CARBON AND OXYGEN.STARRFIELD S; SPARKS WM; TRURAN JW et al.1974; ASTROPHYS. J., SUPPL. SER.; U.S.A.; DA. 1974; VOL. 28; NO 261; PP. 247-270; BIBL. 71 REF.Article

THE EFFECTS OF UNTHERMALIZED ISOMERIC STATES AND OF A TIME-VARYING NEUTRON FLUX ON S-PROCESS BRANCHING RATIOSCOSNER K; IBEN I JR; TRURAN JW et al.1980; ASTROPHYS. J.; USA; DA. 1980; VOL. 238; NO 2 PART. 2; PP. L91-L96; BIBL. 13 REF.Article

CNO ABUNDANCES AND HYDRODYNAMIC MODELS OF THE NOVA OUTBURST. IV. COMPARISON WITH OBSERVATIONS.SPARKS WM; STARRFIELD S; TRURAN JW et al.1976; ASTROPHYS. J.; U.S.A.; DA. 1976; VOL. 208; NO 3 PART. 1; PP. 819-825; BIBL. 41 REF.Article

NOVAE, SUPERNOVAE AND NEUTRONS SOURCES.STARRFIELD S; TRURAN JW; SPARKS WM et al.1975; ASTROPHYS. J.; U.S.A.; DA. 1975; VOL. 198; NO 3 PART. 2; PP. 113-117; BIBL. 11 REF.Article

AN EXTREMELY CARBON ENHANCED "NOVA" MODEL.STARRFIELD SG; SPARKS WM; TRURAN JW et al.1975; MEM. SOC. R. SCI. LIEGE; 8.; BELG.; DA. 1975; VOL. 8; PP. 425-447 (6P.); BIBL. 5 REF.; (PROBL. HYDRODYN. STELLAIRE. 19E. COLLOQ. INT. ASTROPHYS.; LIEGE; 1974)Conference Paper

CNO ABUNDANCES AND HYDRODYNAMIC MODELS OF THE NOVA OUTBURST. III. 0.5 M CERCLE. MODELS WITH ENHANCED CARBON, OXYGEN, AND NITROGEN.STARRFIELD S; SPARKS WM; TRURAN JW et al.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 192; NO 3 PART. 1; PP. 647-655; BIBL. 24 REF.Article

THE AFTERCLAP OF DEGENERATE CARBON IGNITION.BUCHLER JR; MAZUREK TJ; TRURAN JW et al.1974; COMMENTS ASTROPHYS. SPACE PHYS.; U.S.A.; DA. 1974; VOL. 6; NO 2; PP. 45-55; BIBL. 1 P. 1/2Article

EXPLOSIVE HELIUM BURNING IN SUPERNOVAE: A SOURCE OF R-PROCESS ELEMENTSCOWAN JJ; CAMERON AGW; TRURAN JW et al.1983; ASTROPHYSICAL JOURNAL; ISSN 0004-637X; USA; DA. 1983; VOL. 265; NO 1; PART. 1; PP. 429-442; BIBL. 51 REF.Article

THE THERMAN RUNAWAY R-PROCESSCOWAN JJ; CAMERON AGW; TRURAN JW et al.1982; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1982; VOL. 252; NO 1; PART. 1; PP. 348-355; BIBL. 20 REF.Article

A MODEL FOR DWARF NOVAE AS PROGENITORS OF TYPE I SUPERNOVAESTARRFIELD S; TRURAN JW; SPARKS WM et al.1981; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1981; VOL. 243; NO 1; PART. 2; PP. L27-L31; BIBL. 45 REF.Article

THE CAUSE OF THE NOVA OUTBURST.STARRFIELD S; SPARKS WM; TRURAN JW et al.1976; INTERNATION. ASTR. UN., SYMP.; NETHERL.; DA. 1976; NO 73; PP. 155-172; BIBL. 1 P.; (STRUCT. EVOL. CLOSE BINARY SYST. SYMP.; CAMBRIDGE, ENGL.; 1975)Conference Paper

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