Authors:
DENISSENKOV PA
DACOSTA GS
NORRIS JE
WEISS A
Citation: Pa. Denissenkov et al., THE PUZZLING MGAL ANTICORRELATION IN GLOBULAR-CLUSTER RED GIANTS - PRIMORDIAL PLUS DEEP MIXING SCENARIO, Astronomy and astrophysics, 333(3), 1998, pp. 926-941
Citation: Sl. Dupuis et Je. Norris, A MULTIDIMENSIONAL AND CONTEXTUAL FRAMEWORK FOR UNDERSTANDING DIVERSEFAMILY MEMBERS ROLES IN LONG-TERM-CARE FACILITIES, Journal of aging studies, 11(4), 1997, pp. 297-325
Citation: Tc. Beers et al., HIGH-RESOLUTION ABUNDANCE DETERMINATIONS OF EXTREMELY-METAL-POOR STARS AND GALACTIC CHEMICAL EVOLUTION, Nuclear physics. A, 621(1-2), 1997, pp. 37-40
Citation: Je. Norris et al., THE GIANT BRANCH OF OMEGA-CENTAURI - THE DEPENDENCE OF KINEMATICS ON ABUNDANCE, The Astrophysical journal, 487(2), 1997, pp. 187-190
Citation: Sg. Ryan et al., EXTREMELY METAL-POOR STARS .2. ELEMENTAL ABUNDANCES AND THE EARLY CHEMICAL ENRICHMENT OF THE GALAXY, The Astrophysical journal, 471(1), 1996, pp. 254-278
Citation: Je. Norris et al., THE GIANT BRANCH OF OMEGA-CENTAURI .5. THE CALCIUM ABUNDANCE DISTRIBUTION, The Astrophysical journal, 462(1), 1996, pp. 241-254
Citation: Je. Norris et al., EQUIVALENT WIDTHS FOR 54 RED GIANTS IN 47-TUCANAE, OMEGA-CENTAURI, NGC-6397, M22, AND NGC-6752, The Astrophysical journal. Supplement series, 99(2), 1995, pp. 637-658
Citation: Je. Norris et Gs. Dacosta, THE GIANT BRANCH OF OMEGA-CENTAURI .4. ABUNDANCE PATTERNS BASED ON ECHELLE SPECTRA OF 40 RED GIANTS, The Astrophysical journal, 447(2), 1995, pp. 680-705
Citation: Je. Norris et Gs. Dacosta, THE SODIUM ALUMINUM-OXYGEN ANTICORRELATION IN OMEGA-CENTAURI AND OTHER CLUSTERS, The Astrophysical journal, 441(2), 1995, pp. 81-84
Citation: A. Sarajedini et Je. Norris, CCD PHOTOMETRY FOR 6 METAL-RICH GALACTIC GLOBULAR-CLUSTERS, The Astrophysical journal. Supplement series, 93(1), 1994, pp. 161
Citation: Je. Norris, WHY NOT THINK CARNEGIE-HALL - WORKING AND RETIRING AMONG OLDER PROFESSIONALS, Canadian journal on aging, 12(2), 1993, pp. 182-199