kw.\*:("METAL RICH STAR")
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THE EVOLUTION OF SUPER-METAL-RICH STARS AND THE INTERPRETATION OF OLD GALACTIC CLUSTERS.CASTELLANI V; TORNAMBE A.1977; ASTROPHYS. SPACE SCI.; NETHERL.; DA. 1977; VOL. 46; NO 1; PP. 195-203; BIBL. 9 REF.Article
A PROGRESSION IN THE CHARACTERISTICS OF THE PERIOD-AMPLITUDE DIAGRAMS FOR CEPHEIDS IN DIFFERENT GALAXIES.VAN GENDEREN AM.1978; ASTR. AND ASTROPHYS.; GERM.; DA. 1978; VOL. 65; NO 1; PP. 147-149; BIBL. 35 REF.Article
CHROMIUM, MANGANESE, AND IRON IN THE EARLY PECULIAR STARSALLEN MS; COWLEY CR.1977; PUBL. ASTR. SOC. PACIF.; USA; DA. 1977; VOL. 89; NO 529; PP. 386-390; BIBL. 33 REF.Article
LONG-PERIOD VARIABLES IN THE GALACTIC BULGE: EVIDENCE FOR A YOUNG SUPER-METAL-RICH POPULATIONWOOD PR; BESSEL MS.1983; ASTROPHYSICAL JOURNAL; ISSN 0004-637X; USA; DA. 1983; VOL. 265; NO 2; PART. 1; PP. 748-759; BIBL. 54 REF.Article
HD 36619 - A METAL-RICH A-TYPE STAR PREVIOUSLY MISCLASSIFIELD 07WHITTET DCB; KILKENNY D.1979; OBSERVATORY; GBR; DA. 1979; VOL. 99; NO 1028; PP. 4-5; BIBL. 12 REF.Article
IMPLICATIONS OF THE BARIUM ABUNDANCE IN METAL RICH BAII STARSROCCA VOLMERANGE B; AUDOUZE J.1979; ASTR. AND ASTROPHYS.; DEU; DA. 1979; VOL. 75; NO 3; PP. 371-373; BIBL. 27 REF.Article
POSITION DE L'AGE ZERO DE LA SEQUENCE PRINCIPALE POUR DES ETOILES AYANT UNE FORTE ABONDANCE EN METAL SUR LES DIAGRAMMES (MV, B-V), (MV, U-B) ET (U-B, B-V)KHOLOPOV PN.1978; ASTR. CIRK., IZDAV. BJURO ASTR. SOOBSHCH. AKAD. NAUK S.S.S.R.; SUN; DA. 1978; NO 1006; PP. 1-3Article
THE CARBON-TO-IRON RATIO OF METAL-RICH DWARFS: AN ANALYSIS OF 14 HERCULISPETERSON RC.1978; ASTROPHYS. J.; USA; DA. 1978; VOL. 224; NO 2 PART. 1; PP. 595-602; BIBL. 46 REF.Article
A COMPARISON OF TURBULENCE IN NORMAL AND SUPERMETAL-RICH K GIANT STARSGRAY DF; MARTIN BE.1979; ASTROPHYS. J.; USA; DA. 1979; VOL. 231; NO 1 PART. 1; PP. 139-143; BIBL. 12 REF.Article
An R star in the central bulge of the GalaxyEVANS, T. L.Monthly Notices of the Royal Astronomical Society. 1985, Vol 216, Num 2, pp 29P-33P, issn 0035-8711Article
UPPER PHOTOSPHERIC TEMPERATURE MODELS OF K GIANTS: A COMPARISON OF SUPER-METAL-RICH GIANTS WITH NORMAL GIANTSKRISHNA DESIKACHARY; GRAY DF.1978; ASTROPHYS. J.; USA; DA. 1978; VOL. 226; NO 3 PART. 1; PP. 907-922; BIBL. 31 REF.Article
Mu Leonis : the Branch-Bonnell-Tomkin metallicity revisedTAYLOR, B. J.Publications of the Astronomical Society of the Pacific. 1991, Vol 103, Num 667, pp 969-972, issn 0004-6280Article
On the evolutionary status of Mu LeonisHARRIS, M. J; LAMBERT, D. L; SMITH, V. V et al.Publications of the Astronomical Society of the Pacific. 1987, Vol 99, Num 619, pp 1003-1008, issn 0004-6280Article
La Composition chimique des étoiles dans le voisinage solaire : comptes rendus sur les journées de Strasbourg, 7e réunion, Strasbourg, 24 janvier 1985 = Chimical composition of nearby solar stars: report about Strasbourg working days, 7th reunion, Strasbourg, january 24th, 1985La Composition chimique des étoiles dans le voisinage solaire. Journées de Strasbourg. Réunion. 7. 1985, 98 p.Conference Proceedings
Recognition and classification of strong-CN giantsKEENAN, P. C; YORKA, S. B; WILSON, O. C et al.Publications of the Astronomical Society of the Pacific. 1987, Vol 99, Num 617, pp 629-636, issn 0004-6280Article
The alternative X question: what causes the strong molecular bands and damping lines in very strong lined (super―metal-rich) stars?TAYLOR, B. J; JOHNSON, S. B.The Astrophysical journal. 1987, Vol 322, Num 2, pp 930-948, issn 0004-637X, 1Article
A hint on the age and helium content of the Galactic BulgeRENZINI, A.Astronomy and astrophysics (Berlin. Print). 1994, Vol 285, Num 1, pp L5-L8, issn 0004-6361Article
Super-lithium rich starsFARAGGIANA, R; GERBALDI, M; MOLARO, P et al.Memorie della Societa Astronomica Italiana. 1991, Vol 62, Num 1, pp 189-195, issn 0037-8720, 7 p.Article
The nature of the galactic bulgeHARMON, R; GILMORE, G.Lecture notes in physics. 1988, Vol 297, pp 105-108, issn 0075-8450Conference Paper
Theoretical isochrones for old, super-metal-rich starsVANDENBERG, D. A; LASKARIDES, P. G.The Astrophysical journal. Supplement series. 1987, Vol 64, Num 1, pp 103-125, issn 0067-0049Article
ELODIE metallicity-biased search for transiting Hot jupiters. IV. Intermediate period planets orbiting the stars HD 43691 and HD 132406DA SILVA, R; UDRY, S; GALLAND, F et al.Astronomy and astrophysics (Berlin. Print). 2007, Vol 473, Num 1, pp 323-328, issn 0004-6361, 6 p.Article
The N2K consortium. V. Identifying very metal-rich stars with low-resolution spectra : Finding planet-search targetsROBINSON, Sarah E; STRADER, Jay; AMMONS, S. Mark et al.The Astrophysical journal. 2006, Vol 637, Num 2, pp 1102-1112, issn 0004-637X, 11 p., 1Article
ELODIE metallicity-biased search for transiting Hot Jupiters III. A hot Jupiter orbiting the star HD 185269MOUTOU, C; LOEILLET, B; ZUCKER, S et al.Astronomy and astrophysics (Berlin. Print). 2006, Vol 458, Num 1, pp 327-329, issn 0004-6361, 3 p.Article
The metal-rich globular cluster NGC 6553 : clump morphology and ageDEMARQUE, P; LEE, Y.-W.Astronomy and astrophysics (Berlin. Print). 1992, Vol 265, Num 1, pp 40-42, issn 0004-6361Article
IY Hya : a new super Li-rich carbon starABIA, C; BOFFIN, H. M. J; ISERN, J et al.Astronomy and astrophysics (Berlin. Print). 1991, Vol 245, Num 1, pp L1-L4, issn 0004-6361Article