PERIOD CHANGES IN CENTAURUS X-3.SPARKS WM.1975; ASTROPHYS. J.; U.S.A.; DA. 1975; VOL. 199; NO 2 PART. 1; PP. 462-466; BIBL. 44 REF.Article

STUDIES OF HYDRODYNAMIC EVENTS IN STELLAR EVOLUTION. I. METHOD OF COMPUTATIONKUTTER GS; SPARKS WM.1972; ASTROPHYS. J.; U.S.A.; DA. 1972; VOL. 175; NO 2, PART 1; PP. 407-415; BIBL. 21 REF.Serial Issue

STUDIES OF HYDRODYNAMIC EVENTS IN STELLAR EVOLUTION. II. DYNAMIC INSTABILITIES IN STELLAR ENVELOPESSPARKS WM; KUTTER GS.1972; ASTROPHYS. J.; U.S.A.; DA. 1972; VOL. 175; NO 3, PART 1; PP. 707-715; BIBL. 30REF.Serial Issue

STUDIES OF HYDRODYNAMIC EVENTS IN STELLAR EVOLUTION. II. EJECTION OF PLANETARY NEBULAE.KUTTER GS; SPARKS WM.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 192; NO 2 PART. 1; PP. 447-455; BIBL. 29 REF.Article

RADICAL ACCRETION OF H-RICH MATERIAL ONTO A HE WHITE DWARFKUTTER GS; SPARKS WM.1980; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1980; VOL. 239; PP. 988-998; BIBL. 15 REF.Article

A WAVE MODEL FOR DWARF NOVAESPARKS WM; KUTTER GS.1980; SPACE SCI. REV.; ISSN 0038-6308; NLD; DA. 1980; VOL. 27; NO 3-4; PP. 643-648; BIBL. 14 REF.Conference Paper

ON THE LOWER MASS LIMIT FOR THE CARBON DETONATION SCENARIO.ENDAL AS; SPARKS WM.1975; ASTROPHYS. J.; U.S.A.; DA. 1975; VOL. 200; NO 2 PART. 2; PP. 77-78; BIBL. 23 REF.Article

THEORETICAL STUDIES OF MASSIVE STARS. II: EVOLUTION OF A 15 M _CERCLE. STAR FROM CARBON SHELL BURNING TO IRON CORE COLLAPSESPARKS WM; ENDAL AS.1980; ASTROPHYS. J.; USA; DA. 1980; VOL. 237; NO 1 PART. 1; PP. 130-141; BIBL. 34 REF.Article

IS A DWARF NOVA REALLY A "DWARF" NOVA.SPARKS WM; STARRFIELD S.1975; MEM. SOC. R. SCI. LIEGE, 8.; BELG.; DA. 1975; VOL. 8; PP. 407-447 (7P.); BIBL. 13 REF.; (PROBL. HYDRODYN. STELLAIRE. 19E. COLLOQ. INT. ASTROPHYS.; LIEGE; 1974)Conference Paper

DEATH THROES OF MASSIVE STARSSOFIA S; SPARKS WM; FENDAL AS et al.1979; NATURE; GBR; DA. 1979; VOL. 277; NO 5696; PP. 456-457; BIBL. 11 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

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

LOS ALAMOS/GODDARD CONFERENCE CURRENT PROBLEMS IN STELLAR PULSATION INSTABILITIESLESH JR; SPARKS WM; FISCHEL D et al.1979; COMMENTS OU ASTROPHYS.; GBR; DA. 1979; VOL. 8; NO 5; PP. 151-162Article

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

ACCRETION AND THE NOVA OUTBURST.STARRFIELD SG; SPARKS WM; TRURAN JW et al.1975; MEM. SOC. R. SCI. LIEGE; 8.; BELG.; DA. 1975; VOL. 8; PP. 413-447 (13P.); BIBL. 8 REF.; (PROBL. HYDRODYN. STELLAIRE. 19E. COLLOQ. INT. ASTROPHYS.; LIEGE; 1974)Conference Paper

PHOTOMETRIC CALIBRATION OF THE INTERNATIONAL ULTRAVIOLET EXPLORER (IUE): LOW DISPERSIONBOHLIN RC; HOLM AV; SAVAGE BD et al.1980; ASTR. AND ASTROPHYS.; DEU; DA. 1980; VOL. 85; NO 1-2; PP. 1-13; BIBL. 21 REF.Article

ON INTERSTELLAR ACCRETION AND THE REJUVENATION OF WHITE DWARFS.TRURAN JW; STARRFIELD SG; STRITTMATTER PA et al.1977; ASTROPHYS. J.; U.S.A.; DA. 1977; VOL. 211; NO 2 PART. 1; PP. 539-546; BIBL. 29 REF.Article

CNO ABUNDANCES AND HYDRODYNAMIC MODELS OF THE NOVA OUTBURSTSTARRFIELD S; TRURAN JW; SPARKS WM et al.1972; ASTROPHYS. J.; U.S.A.; DA. 1972; VOL. 176; NO 1, PART 1; PP. 169-176; BIBL. 17REF.Serial Issue

THERMONUCLEAR PROCESSES AND ACCRETION ONTO NEUTRON STAR ENVELOPES: X-RAY BURST AND TRANSIENT SOURCESSTARRFIELD S; KENYON S; SPARKS WM et al.1982; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1982; VOL. 258; NO 2; PART. 1; PP. 683-695; BIBL. 48 REF.Article