Pascal and Francis Bibliographic Databases

Help

Search results

Your search

au.\*:("ARNETT WD")

Document Type [dt]

A-Z Z-A Frequency ↓ Frequency ↑
Export in CSV

Publication Year[py]

A-Z Z-A Frequency ↓ Frequency ↑
Export in CSV

Results 1 to 25 of 47

  • Page / 2
Export

Selection :

  • and

NEUTRINO TRAPPING DURING GRAVITATIONAL COLLAPSE OF STARS.ARNETT WD.1977; ASTROPHYS. J.; U.S.A.; DA. 1977; VOL. 218; NO 3 PART. 1; PP. 815-833; BIBL. 48 REF.Article

SUPERNOVAE AS PHENOMENA OF HIGH-ENERGY ASTROPHYSICS.ARNETT WD.1977; ANN. NEW YORK ACAD. SCI.; U.S.A.; DA. 1977; VOL. 302; PP. 90-100; BIBL. 44 REF.; (TEXAS SYMP. RELATIV. ASTROPHYS. 8; BOSTON; 1976)Conference Paper

NUCLEAR REACTIONS AND NEUTRINOS IN STELLAR EVOLUTION.ARNETT WD.1974; INTERNATION. ASTR. UN., SYMP.; NETHERL.; DA. 1974; NO 66; PP. 1-255 (17P.); BIBL. DISSEM.; (LATE STAGES STELLAR EVOL. COPERNICUS SYMP. V; WARSAW; 1973)Conference Paper

THE COSMIC DISTANCE SCALE: METHODS FOR DETERMINING THE DISTANCE TO SUPERNOVAEARNETT WD.1982; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1982; VOL. 254; NO 1; PART. 1; PP. 1-7; BIBL. 21 REF.Article

TYPE I SUPERNOVAE. I: ANALYTIC SOLUTIONS FOR THE EARLY PART OF THE LIGHT CURVEARNETT WD.1982; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1982; VOL. 253; NO 2; PART. 1; PP. 785-797; BIBL. 27 REF.Article

ON THE BULK YIELDS OF NUCLEOSYNTHESIS FROM MASSIVE STARSARNETT WD.1978; ASTROPHYS. J.; USA; DA. 1978; VOL. 219; NO 3 PART. 1; PP. 1008-1016; BIBL. 1/2 P.Article

ON THE THEORY OF TYPE I SUPERNOVAEARNETT WD.1979; ASTROPHYS. J.; USA; DA. 1979; VOL. 230; NO 1 PART. 2; PP. L37-L40; BIBL. 36 REF.Article

ADVANCED EVOLUTION OF MASSIVE STARS. VII. SILICON BURNING.ARNETT WD.1977; ASTROPHYS. J., SUPPL. SER.; U.S.A.; DA. 1977; VOL. 35; NO 2; PP. 145-159; BIBL. 30 REF.Article

GAMMA RAYS AND SUPERNOVA EXPLOSIONS.ARNETT WD.sdIN: STRUCT. CONTENT GALAXY GALACTIC GAMMA RAYS. INT. SYMP. PROC.; GREENBELT, MD.; 1976; GREENBELT, MD.; TECH. INF. DIV.; DA. S.D.; PP. 289-298; BIBL. 12 REF.Conference Paper

HYDROSTATIC OXYGEN BURNING IN STARS. I. OXYGEN STARSARNETT WD.1972; ASTROPHYS. J.; U.S.A.; DA. 1972; VOL. 17; NO 2, PART 1; PP. 393-400; BIBL. 10 REF.Serial Issue

NEUTRINO ESCAPE, NUCLEAR DISSOCIATION, AND CORE COLLAPSE AND/OR EXPLOSIONARNETT WD.1982; ASTROPHYSICAL JOURNAL; ISSN 0004-637X; USA; DA. 1982; VOL. 263; NO 2; PART. 2; PP. L55-L57; BIBL. 19 REF.Article

NEUTRONIZATION, LEPTON ESCAPE, AND STELLAR HYDRODYNAMICSARNETT WD.1980; J. PHYS., COLLOQ.; FRA; DA. 1980; NO 2; PP. 25-29; ABS. FRE; BIBL. 18 REF.Conference Paper

ANALYTIC SOLUTIONS FOR LIGHT CURVES OF SUPERNOVAE OF TYPE IIARNETT WD.1980; ASTROPHYS. J.; USA; DA. 1980; VOL. 237; NO 2 PART. 1; PP. 541-549; BIBL. 15 REF.Article

SUPERNOVA REMNANTS AND PRESUPERNOVA MODELS.ARNETT WD.1975; ASTROPHYS. J.; U.S.A.; DA. 1975; VOL. 195; NO 3 PART. 1; PP. 727-733; BIBL. 43 REF.Article

IRON PRODUCTION BY 12C-DETONATION SUPERNOVAE.ARNETT WD.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 191; NO 3 PART. 1; PP. 727-729; BIBL. 19 REF.Article

ADVANCED EVOLUTION OF MASSIVE STARS. V. NEON BURNING.ARNETT WD.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 193; NO 1 PART. 1; PP. 169-176; BIBL. 21 REF.Article

NONUNIFORM ABUNDANCES IN YOUNG SUPERNOVA REMNANTSARNETT WD.1980; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1980; VOL. 240; NO 1; PART. 1; PP. 105-108; BIBL. 27 REF.Article

ADVANCED EVOLUTION OF MASSIVE STARS. I. HELIUM BURNINGARNETT WD.1972; ASTROPHYS. J.; U.S.A.; DA. 1972; VOL. 176; NO 3, PART 1; PP. 681-698; BIBL. 31REF.Serial Issue

ADVANCED EVOLUTION OF MASSIVE STARS. II. CARBON BURNINGARNETT WD.1972; ASTROPHYS. J.; U.S.A.; DA. 1972; VOL. 176; NO 3, PART 1; PP. 699-710; BIBL. 32REF.Serial Issue

RADIATION DYNAMICS, ENVELOPE EJECTION, AND SUPERNOVA LIGHT CURVES.FALK SW; ARNETT WD.1977; ASTROPHYS. J., SUPPL. SER.; U.S.A.; DA. 1977; VOL. 33; NO 4; PP. 515-562; BIBL. 1 P.Article

ADVANCED EVOLUTION OF MASSIVE STARS. IV. SECONDARY NUCLEOSYNTHESIS DURING HELIUM BURNINGCOUCH RG; ARNETT WD.1972; ASTROPHYS. J.,; U.S.A.; DA. 1972; VOL. 178; NO 3, PART1; PP. 771-777; BIBL. 17REF.Serial Issue

ORIGIN OF COSMIC RAYS IN EXPLOSIONS OF MASSIVE STARS.SCHRAMM DN; ARNETT WD.sdIN: 13TH INT. COSMIC RAY CONF.; DENVER, COLO.; 1973; DENVER, COLO.; UNIV. DENVER; DA. S.D.; VOL. 1; PP. 646-651; BIBL. 1 P.Conference Paper

ALUMINIUM-26 PRODUCTION FROM A STELLAR EVOLUTIONARY SEQUENCE.ARNETT WD; WEFEL JP.1978; ASTROPHYS. J.; USA; DA. 1978; VOL. 224; NO 3 PART. 2; PP. L139-L142; BIBL. 27 REF.Article

NUMERICAL STUDIES OF NONSPHERICAL CARBON COMBUSTION MODELSMUELLER E; ARNETT WD.1982; ASTROPHYSICAL JOURNAL; ISSN 0004-637X; USA; DA. 1982; VOL. 261; NO 2; PART. 2; PP. L109-L115; BIBL. 18 REF.Article

A MICROSCOPIC INTERPRETATION OF NEUTRON STAR STRUCTURE.ARNETT WD; BOWERS RL.1977; ASTROPHYS. J., SUPPL. SER.; U.S.A.; DA. 1977; VOL. 33; NO 4; PP. 415-436; BIBL. 58 REF.Article

  • Page / 2