COMMENT ON THE QUARK BURNING MODEL OF QUASARS.TOIYA T; TERASAKI K.1974; PROGR. THEOR. PHYS.; JAP.; DA. 1974; VOL. 52; NO 2; PP. 713-715; BIBL. 6 REF.Article

DUST MODELS FOR INFRARED GALAXIESWICKRAMASINGHE NC.1972; MEM. SOC. R. SCI. LIEGE, 8O; )BELG.; DA. 1972; VOL. 3; PP. 601-629 (7 P.); BIBL. 7 REF.Serial Issue

NEUTRINO PROCESSES AND QSOS.TENNAKONE K.1975; NATURE; G.B.; DA. 1975; VOL. 254; NO 5499; PP. 399-400; BIBL. 4 REF.Article

MODELS WITH PARTICLE-HOLE SYMMETRY AND SINGULAR COEXISTENCE-CURVE DIAMETERSREHR JJ; MERMIN ND.1973; PHYS. REV., A; U.S.A.; DA. 1973; VOL. 7; NO 1; PP. 379-380; BIBL. 6 REF.Serial Issue

AN EXACT SOLUTION FOR A COLLISIONLESS FLAT GALACTIC MODELAOKI S.1973; PUBL. ASTR. SOC. JAP.; JAP.; DA. 1973; VOL. 25; NO 1; PP. 35-50; BIBL. 10 REF.Serial Issue

MODELES THEORIQUES D'ERUPTIONSSYROVATSKIJ SI.1973; VEST. AKAD. NAUK S.S.S.R.; S.S.S.R.; DA. 1973; NO 3; PP. 31-36Serial Issue

THE STRUCTURE OF PULSAR MAGNETOSPHERES1972; ASTROPHYS. J.; U.S.A.; DA. 1972; VOL. 173; NO 1 PART 2; PP. 33-37; BIBL. 18REF.Serial Issue

A TWIN-EXHAUST MODEL FOR DOUBLE RADIO SOURCES.BLANDFORD RD; REES MJ.1974; MONTH. NOT. R. ASTR. SOC.; G.B.; DA. 1974; VOL. 169; NO 3; PP. 395-415; BIBL. 41 REF.Article

CONFIGURATION OF THE JOVIAN MAGNETOSPHERE.HILL TW; DESSLER AJ; MICHEL FC et al.1974; GEOPHYS. RES. LETTERS; U.S.A.; DA. 1974; VOL. 1; NO 1; PP. 3-6; BIBL. 11 REF.Article

MATHEMATICAL MODELING IN THE DESIGN OF FLUID POWER SYSTEMS.REID KN; BOSE JE.1974; IN: FLOW. MEAS. CONTROL IN SCI. IND. SYMP. 1. PROC.; PITTSBURGH, PA.; 1971; PITTSBURGH; INSTRUM. SOC. AM.; DA. 1974; PP. 1191-1195; BIBL. 6 REF.Conference Paper

A NOTE ON THE MECHANICS OF OVULATIONLARDNER TJ; SHACK WJ; TAM PY et al.1974; J. THEOR. BIOL.; U.S.A.; DA. 1974; VOL. 48; NO 2; PP. 481-483; BIBL. 5REF.Article

EMISSION MECHANISM IN PULSARSSMITH FG.1973; NATURE; G.B.; DA. 1973; VOL. 243; NO 5404; PP. 207-210; BIBL. 15REF.Serial Issue

LOW MASS B STARS WITH LOW SURFACE GRAVITYTRIMBLE V.1973; ASTR. AND ASTROPHYS.; GERM.; DA. 1973; VOL. 23; NO 2; PP. 281-283; BIBL. 8 REF.Serial Issue

NATURE OF CYGNUS X-3BRUHWEILER F.1973; NATURE PHYS. SCI.; G.B.; DA. 1973; VOL. 244; NO 135; PP. 68-69; BIBL. 5REF.Serial Issue

CRATERS FORMED IN MINERAL DUST BY HYPERVELOCITY MICROPARTICLESVEDDER JF.1972; J. GEOPHYS. RES.; U.S.A.; DA. 1972; VOL. 77; NO 23; PP. 4304-4309; BIBL. 21REF.Serial Issue

SPATIAL SPECTROSCOPIC DIAGNOSTIC OF PLANETARY NEBULAE. III. NUMERICAL INVESTIGATION OF LOCAL ABSOLUTE MONOCHROMATIC ENERGIES AND LOCAL ABSOLUE ENERGIES IN SPHERICALLY SYMMETRIC MODELSHEKELA J; HUBENY I.1972; BULL. ASTR. INST. CZECHOSL.,; CZECHOSL.; DA. 1972; VOL. 23; NO 6; PP. 331-341; ABS. RUSSE; BIBL. 2REF.Serial Issue

UEBER DEN AUFBAU VON 11 OFFENEN STERNHAUGEN = STRUCTURE DE 11 AMAS OUVERTSLOHMANN W.1972; ASTR. NACHR.; DTSCH.; DA. 1972; VOL. 294; NO 3; PP. 105-111; ABS. ANGL.; BIBL. 8 REF.Serial Issue

ACTIVITY IN GALAXIES AND QUASARSSTURROCK PA; BARNES C.1972; ASTROPHYS. J.; U.S.A.; DA. 1972; VOL. 176; NO 1, PART 1; PP. 31-45; BIBL. 1P.Serial Issue

Effet d'une digue sur l'écoulement d'un aérosol = Effect of a dam on a powder snow avalancheAUGE, A; OUSSET, F; MARCO, O et al.Les apports de la recherche scientifique à la sécurité neige glace et avalanche. 1995, 5 p.Conference Paper

BUBBLE MODEL OF EXTRAGALACTIC RADIO SOURCESGULL SF; NORTHOVER KJE.1973; NATURE; G.B.; DA. 1973; VOL. 244; NO 5411; PP. 80-83; BIBL. 19REF.Serial Issue

FURTHER EVIDENCE FOR A BLACK HOLE IN BETA LYRAE.KONDO Y; MCCLUSKEY GE JR; HOUCK TE et al.1972; NATURE PHYS. SCI.; G.B.; DA. 1972; VOL. 240; NO 101; PP. 119-120; BIBL. 7REF.Serial Issue

ORBIT-ORBIT RESONANCE CAPTURE IN THE SOLAR SYSTEMGREENBERG RJ; COUNSELMAN CC III; SHAPIRO II et al.1972; SCIENCE,; U.S.A.; DA. 1972; VOL. 178; NO 4062; PP. 747-749; BIBL. 6REF.Serial Issue

THE INFRARED VARIABILITY OF A DUST MODEL FOR SEYFERT GALAXIESKANEKO N; TOYAMA K; NISHIMURA M et al.1972; ASTROPHYS. SPACE SCI.,; NETHERL.; DA. 1972; VOL. 18; NO 1; PP. 121-127; BIBL. 12REF.Serial Issue

MODELE DU SYSTEME BETA LYR1972; ASTR. CIRK., IZDAV. BJURO ASTR. SOOBSHCH. AKAD. NAUK S.S.S.R.; S.S.S.R.; DA. 1972; NO 707; PP. 1-3; BIBL. 11REF.Serial Issue

QUELQUES CONSEQUENCES OBSERVATIONNELLES DU MODELE DE FORMATION DES GALAXIES PAR PERTURBATIONS ADIABATIQUESNARITS AD.1972; ASTR. CIRK., IZDAV. BJURO ASTR. SODSSHCH. AKAD. NAUK S.S.S.R.; S.S.S.R.; DA. 1972; NO 732; PP. 5-7; BIBL. 7REF.Serial Issue