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Results: 1-25 |
Results: 25

Authors: MOWLAVI N SCHAERER D MEYNET G BERNASCONI PA
Citation: N. Mowlavi et al., GRIDS OF STELLAR MODELS - VII - FROM 0.8 TO 60 M-CIRCLE-DOT AT Z = 0.10, Astronomy & Astrophysics. Supplement series, 128(3), 1998, pp. 471-474

Authors: KIENZLE F BURKI G BURNET M MEYNET G
Citation: F. Kienzle et al., THE PULSATING YELLOW SUPERGIANT V810 CENTAURI, Astronomy and astrophysics (Berlin), 337(3), 1998, pp. 779-789

Authors: MOWLAVI N MEYNET G MAEDER A SCHAERER D CHARBONNEL C
Citation: N. Mowlavi et al., ON SOME PROPERTIES OF VERY METAL-RICH STARS, Astronomy and astrophysics (Berlin), 335(2), 1998, pp. 573-582

Authors: SCHAERER D CONTINI T KUNTH D MEYNET G
Citation: D. Schaerer et al., DETECTION OF WOLF-RAYET STARS OF WN AND WC SUBTYPES IN SUPERSTAR CLUSTERS OF NGC-5253, The Astrophysical journal, 481(2), 1997, pp. 75-79

Authors: TALON S ZAHN JP MAEDER A MEYNET G
Citation: S. Talon et al., ROTATIONAL MIXING IN EARLY-TYPE STARS - THE MAIN-SEQUENCE EVOLUTION OF A 9-M-CIRCLE-DOT STAR, Astronomy and astrophysics, 322(1), 1997, pp. 209-217

Authors: ARNOULD M PAULUS G MEYNET G
Citation: M. Arnould et al., SHORT-LIVED RADIONUCLIDE PRODUCTION BY NON-EXPLODING WOLF-RAYET STARS, Astronomy and astrophysics, 321(2), 1997, pp. 452-464

Authors: MEYNET G MAEDER A
Citation: G. Meynet et A. Maeder, STELLAR EVOLUTION WITH ROTATION .1. THE COMPUTATIONAL METHOD AND THE INHIBITING EFFECT OF THE MU-GRADIENT, Astronomy and astrophysics, 321(2), 1997, pp. 465-476

Authors: MEYNET G ARNOULD M PRANTZOS N PAULUS G
Citation: G. Meynet et al., CONTRIBUTION OF WOLF-RAYET STARS TO THE SYNTHESIS OF AL-26 .1. THE GAMMA-RAY CONNECTION, Astronomy and astrophysics, 320(2), 1997, pp. 460-468

Authors: CHARBONNEL C MEYNET G MAEDER A SCHAERER D
Citation: C. Charbonnel et al., GRIDS OF STELLAR MODELS .6. HORIZONTAL-BRANCH AND EARLY ASYMPTOTIC GIANT BRANCH FOR LOW-MASS STARS (Z=0.020, 0.001), Astronomy & Astrophysics. Supplement series, 115(2), 1996, pp. 339-344

Authors: MAEDER A MEYNET G
Citation: A. Maeder et G. Meynet, DIFFUSIVE MIXING BY SHEARS IN ROTATING STARS, Astronomy and astrophysics, 313(1), 1996, pp. 140-144

Authors: LEITHERER C ALLOIN D FRITZVONALVENSLEBEN U GALLAGHER JS HUCHRA JP MATTEUCCI F OCONNELL RW BECKMAN JE BERTELLI GP BICA E BOISSON C BONATTO C BOTHUN GD BRESSAN A BRODIE JP BRUZUAL G BURSTEIN D BUSER R CALDWELL N CASUSO E CERVINO M CHARLOT S CHAVEZ M CHIOSI C CHRISTIAN CA CUISINIER F DALLIER R DEKOTER A DELISLE S DIAZ AI DOPITA MA DORMAN B FAGOTTO F FANELLI MN FIOC M GARCIAVARGAS ML GIRARDI L GOLDADER JD HARDY E HECKMAN TM IGLESIAS J JABLONKA P JOLY M JONES L KURTH O LANCON A LEJEUNE T LOXEN J MAEDER A MALAGNINI ML MARIGO P MASHESSE JM MEYNET G MOLLER CS MOLLA ML MOROSSI C NASI E NICHOLS JS ODEGAARD KJR PARKER JWM PASTORIZA MG PELETIER R ROBERT C ROCCAVOLMERANGE B SCHAERER D SCHMIDT A SCHMITT HR SCHOMMER RA SCHMUTZ W ROOS MS SILVA L STASINSKA G SUTHERLAND RS TANTALO R TRAAT P VALLENARI A VAZDEKIS A WALBORN NR WORTHEY G WU CC
Citation: C. Leitherer et al., A DATA-BASE FOR GALAXY EVOLUTION MODELING, Publications of the Astronomical Society of the Pacific, 108(729), 1996, pp. 996-1017

Authors: MEYNET G
Citation: G. Meynet, WOLF-RAYET POPULATION SYNTHESES FOR STARBURST GALAXIES, Astronomy and astrophysics, 298(3), 1995, pp. 767-783

Authors: MEYNET G
Citation: G. Meynet, HOT PAPERS - ASTROPHYSICS - NEW GRIDS OF STELLAR MODELS FROM 0.8 TO 120M-CIRCLE-DOT AT Z=0.020 AND Z=0.001 - SCHALLER,G., SCHAERER,D., MEYNET,G., MAEDER,A., The Scientist, 8(20), 1994, pp. 16-16

Authors: MEYNET G MAEDER A SCHALLER G SCHAERER D CHARBONNEL C
Citation: G. Meynet et al., GRIDS OF MASSIVE STARS WITH HIGH-MASS LOSS RATES .5. FROM 12 TO 120 M(CIRCLE-DOT) AT Z=0.001, 0.004, 0.008, 0.020 AND 0.040, Astronomy & Astrophysics. Supplement series, 103(1), 1994, pp. 97-105

Authors: MEYNET G
Citation: G. Meynet, OBSERVATION OF THE 1.8 MEV EMISSION-LINE FROM AL-26 AND THE CHEMICAL EVOLUTION OF THE GALAXY, The Astrophysical journal. Supplement series, 92(2), 1994, pp. 441-447

Authors: MAEDER A MEYNET G
Citation: A. Maeder et G. Meynet, NEW MODELS OF WOLF-RAYET STARS AND COMPARISON WITH DATA IN GALAXIES, Astronomy and astrophysics, 287(3), 1994, pp. 803-816

Authors: SMITH LF MEYNET G MERMILLIOD JC
Citation: Lf. Smith et al., IMPROVED BOLOMETRIC CORRECTIONS FOR WR STARS FROM CLUSTER MEMBERSHIP AND EVOLUTIONARY MODELS, Astronomy and astrophysics, 287(3), 1994, pp. 835-842

Authors: CHARBONNEL C VAUCLAIR S MAEDER A MEYNET G SCHALLER G
Citation: C. Charbonnel et al., LITHIUM AND BERYLLIUM DEPLETION BY ROTATION-INDUCED MIXING IN THE SUNAND IN GALACTIC CLUSTER STARS, Astronomy and astrophysics, 283(1), 1994, pp. 155-162

Authors: MEYNET G MERMILLIOD JC MAEDER A
Citation: G. Meynet et al., NEW DATING OF GALACTIC OPEN CLUSTERS, Astronomy & Astrophysics. Supplement series, 98(3), 1993, pp. 477-504

Authors: SCHAERER D MEYNET G MAEDER A SCHALLER G
Citation: D. Schaerer et al., GRIDS OF STELLAR MODELS .2. FROM 0.8 TO 120 M-CIRCLE-DOT AT Z = 0.008, Astronomy & Astrophysics. Supplement series, 98(3), 1993, pp. 523-527

Authors: SCHAERER D CHARBONNEL C MEYNET G MAEDER A SCHALLER G
Citation: D. Schaerer et al., GRIDS OF STELLAR MODELS .4. FROM 0.8 TO 120 M(CIRCLE-DOT) AT Z=0.040, Astronomy & Astrophysics. Supplement series, 102(2), 1993, pp. 339-342

Authors: CHARBONNEL C MEYNET G MAEDER A SCHALLER G SCHAERER D
Citation: C. Charbonnel et al., GRIDS OF STELLAR MODELS .3. FROM 0.8 TO 120-M-CIRCLE-DOT AT Z = 0.004, Astronomy & Astrophysics. Supplement series, 101(2), 1993, pp. 415-419

Authors: SMITH LF MEYNET G MERMILLIOD JC
Citation: Lf. Smith et al., IMPROVED BOLOMETRIC CORRECTIONS FOR WR STARS, Space science reviews, 66(1-4), 1993, pp. 413-416

Authors: MEYNET G
Citation: G. Meynet, WOLF-RAYET STARS IN STARBURSTS - EFFECTS OF AGE AND METALLICITY, Space science reviews, 66(1-4), 1993, pp. 417-420

Authors: MAEDER A MEYNET G
Citation: A. Maeder et G. Meynet, ISOTOPIC ANOMALIES IN COSMIC-RAYS AND THE METALLICITY GRADIENT IN THEGALAXY, Astronomy and astrophysics, 278(2), 1993, pp. 406-414
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