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THE C/N RATIO AND N14 ABUNDANCE AS TESTS OF THE THEORIES OF WOLF-RAYET STARS FORMATIONGABRIEL M; NOELS A.1981; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1981; VOL. 94; NO 1; PP. L1-L2; BIBL. 9 REF.Article

VIBRATIONAL STABILITY AND CRITICAL MASS OF THE STARSNOELS A; MASEREEL C.1982; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1982; VOL. 105; NO 2; PP. 293-295; BIBL. 16 REF.Article

ON THE POSSIBILITY OF CONTAMINATION OF THE SOLAR SURFACE BY ACCRETION.GABRIEL M; NOELS A.1977; ASTR. AND ASTROPHYS.; GERM.; DA. 1977; VOL. 59; NO 3; PP. 427-431; BIBL. 7 REF.Article

INFLUENCE OF THE VARIATION OF THE CONVECTIVE ZONE BOUNDARIES ON THE SECULAR STABILITY OF STARS.GABRIEL M; NOELS A.1974; ASTR. AND ASTROPHYS.; GERM.; DA. 1974; VOL. 34; NO 3; PP. 455-456; BIBL. 3 REF.Article

SECULAR STABILITY OF STATIC MODELS DURING CENTRAL HELIUM BURNINGGABRIEL M; NOELS A.1973; ASTR. AND ASTROPHYS.; GERM.; DA. 1973; VOL. 25; NO 2; PP. 313-317; BIBL. 15REF.Serial Issue

SEMICONVECTION IN STARS OF ABOUT 1M CERCLE..GABRIEL M; NOELS A.1977; ASTR. AND ASTROPHYS.; GERM.; DA. 1977; VOL. 54; NO 2; PP. 631-634; BIBL. 6 REF.Article

ON THE CONDITIONS FOR HOMOGENEOUS STELLAR MODELS TO HAVE ONLY REAL SECULAR EIGENVALUESGABRIEL M; NOELS A.1972; ASTR. AND ASTROPHYS.; GERM.; DA. 1972; VOL. 20; NO 3; PP. 455-459; BIBL. 13REF.Serial Issue

SECULAR STABILITY OF AN 8 M STAR DURING CENTRAL HELIUM BURNINGNOELS A; GABRIEL M.1973; ASTR. AND ASTROPHYS.; GERM.; DA. 1973; VOL. 24; NO 2; PP. 201-208; BIBL. 11REF.Serial Issue

NON-RADIAL SECULAR STABILITY OF THE HYDROGEN BURNING SHELL IN STARS OF 1.1 M CERCLE. AND 8 M CERCLE..GABRIEL M; NOELS A.1976; ASTR. AND ASTROPHYS.; GERM.; DA. 1976; VOL. 46; NO 2; PP. 313-316; BIBL. 7 REF.Article

STABILITY OF A 30 M CERCLE. STAR TOWARDS G+ MODES OF HIGH SPHERICAL HARMONIC VALUES.GABRIEL M; NOELS A.1976; ASTR. AND ASTROPHYS.; GERM.; DA. 1976; VOL. 53; NO 1; PP. 149-157; BIBL. 22 REF.Article

TRANSITION METALS CATALYSED REARRANGEMENTS OF BETA -LACTONESNOELS A; LEFEBVRE P.1973; TETRAHEDRON LETTERS; G.B.; DA. 1973; NO 32; PP. 3035-3038; BIBL. 5 REF.Serial Issue

EVOLUTION OF MASSIVE STARS WITH MASS LOSS AND FORMATION OF WR STARSNOELS A; GABRIEL M.1981; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1981; VOL. 101; NO 2; PP. 215-222; BIBL. 38 REF.Article

THE SOLAR STRUCTURE AND THE LOW L FIVE-MINUTE OSCILLATION. IGABRIEL M; SCUFLAIRE R; NOELS A et al.1982; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1982; VOL. 110; NO 1; PP. 50-53; BIBL. 21 REF.Article

INFLUENCE OF THE EQUATIONS OF STATE AND OF THE Z VALUE ON THE SOLAR FIVE-MINUTE OSCILLATIONSHIBAHASHI H; NOELS A; GABRIEL M et al.1983; ASTRONOMY AND ASTROPHYSICS; ISSN 0004-6361; DEU; DA. 1983; VOL. 123; NO 2; PP. 283-288; BIBL. 25 REF.Article

VIBRATIONAL INSTABILITY OF A 3000 M CERCLE. STAR AND THE R 136A PROBLEMLEDOUX P; NOELS A; BOURY A et al.1982; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1982; VOL. 108; NO 1; PP. 49-50; BIBL. 19 REF.Article

VIBRATIONAL STABILITY OF FIRST GENERATION STARSIBRAHIM A; BOURY A; NOELS A et al.1981; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1981; VOL. 103; NO 2; PP. 390-392; BIBL. 15 REF.Article

STABILITE VIBRATIONNELLE D'UNE ETOILE DE CARBONE DE 0.8M AU COURS DU FLASH DE CARBONECHANMUGAM G; NOELS A; GABRIEL M et al.1972; BULL. SOC. R. SCI. LIEGE; BELG.; DA. 1972; VOL. 41; NO 11-12; PP. 694-699; ABS. ANGL.; BIBL. 6REF.Serial Issue

THE SOLAR STRUCTURE AND THE LOW 1 FIVE-MINUTE OSCILLATION. IISCUFLAIRE R; GABRIEL M; NOELS A et al.1982; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1982; VOL. 113; NO 2; PP. 219-222; BIBL. 11 REF.Article

THE SOLAR STRUCTURE AND THE FIVE-MINUTE OSCILLATIONSCUFLAIRE R; GABRIEL M; NOELS A et al.1981; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1981; VOL. 99; NO 1; PP. 39-42; BIBL. 24 REF.Article

STABILITY OF G+ MODES IN A 30 M CERCLE. STAR.GABRIEL M; NOELS A; SCUFLAIRE R et al.1975; MEM. SOC. R. SCI. LIEGE, 8.; BELG.; DA. 1975; VOL. 8; PP. 273-308 (16P.); BIBL. 8 REF.; (PROBL. HYDRODYN. STELLAIRE. 19E. COLLOQ. INT. ASTROPHYS.; LIEGE; 1974)Conference Paper

INFLUENCE DE LA CONVECTION SUR LA STABILITE DES OSCILLATIONS NON RADIALES DES ETOILES.GABRIEL M; SCUFLAIRE R; NOELS A et al.1974; ACAD. R. BELG., BULL. CL. SCI.; BELG.; DA. 1974; VOL. 60; NO 7; PP. 866-887; ABS. ANGL.; BIBL. 7 REF.Article

NON-RADIAL OSCILLATIONS OF A 1 M CERCLE. STAR WITH AN INITIAL DISCONTINUITY IN CHEMICAL COMPOSITIONBOURY A; SCUFLAIRE R; NOELS A et al.1980; ASTR. AND ASTROPHYS.; DEU; DA. 1980; VOL. 85; NO 1-2; PP. 20-25; BIBL. 23 REF.Article

VIBRATIONAL STABILITY TOWARDS NON-RADIAL OSCILLATIONS DURING CENTRAL HYDROGEN BURNING.NOELS A; BOURY A; GABRIEL M et al.1976; ASTR. AND ASTROPHYS.; GERM.; DA. 1976; VOL. 49; NO 1; PP. 103-106; BIBL. 10 REF.Article

VIBRATIONAL STABILITY OF G+ MODES TOWARDS NON-RADIAL OSCILLATIONS FOR SOLAR MODELS.NOELS A; GABRIEL M; BOURY A et al.1975; MEM. SOC. R. SCI. LIEGE, 8.; BELG.; DA. 1975; VOL. 8; PP. 317-325 (8P.); BIBL. 13 REF.; (PROBL. HYDRODYN. STELLAIRE. 19E. COLLOQ. INT. ASTROPHYS.; LIEGE; 1974)Conference Paper

Trapped non-radial oscillation modes in Wolf-Rayet modelsSCUFLAIRE, R; NOELS, A.Astronomy and astrophysics (Berlin. Print). 1986, Vol 169, Num 1-2, pp 185-188, issn 0004-6361Article

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