Metal-Rich Fused Clusters: Syntheses, Structures, and Bonding of Heteronuclear Condensed Metallaboranes

被引:0
|
作者
Jaiswal, Shippy [1 ]
Pradhan, Alaka Nanda [1 ]
Ghosh, Sundargopal [1 ]
机构
[1] Indian Inst Technol Madras, Dept Chem, Chennai 600036, India
关键词
CHEMISTRY; COMPLEXES; CUBANE;
D O I
10.1021/acs.organomet.4c00288
中图分类号
O61 [无机化学];
学科分类号
070301 ; 081704 ;
摘要
Syntheses and structural elucidations of a series of condensed clusters are described. The condensation of nido-[(Cp*Ru)(2)(B3H9)], nido-1, with heavier group 7 metal carbonyl, [Re-2(CO)(10)], yielded [(Cp*Ru)(2)(CO)B3H8{Re(CO)(3)}], 2. Ruthenaborane 2 is an edge-fused cluster of square pyramid {RuReB3} and triangle {RuB2} through a B-B bond. Further, the reaction of arachno-[(Cp*Ru)(2)(B3H8)(CS2H)], arachno-3, with [Co-2(CO)(8)] led to the formation of condensed ruthenaboranes [(Cp*Ru)(2)B3H3S{Co-3(CO)(8)}(SCH3)], 4, and [(Cp*Ru)(2)B3H4{Co-2(CO)(7)}(SCH3)], 5. Cluster 4 comprises two tetrahedron {Co2RuB}, {Co2BS} and pentagonal pyramidal {Co2RuB3} cores, and cluster 5 consists of a butterfly {Ru2B2}, a triangle {CoB2}, and a tetrahedron {Co2B2}. Both clusters 4 and 5 do not follow Mingos' fusion formalism for fused clusters and are unusual examples based on their composition. On the other hand, cluster 2 follows Mingos' fusion formalism. All of the clusters have been characterized by H-1, B-11{H-1}, C-13{H-1} NMR spectroscopies, electrospray ionization (ESI) mass spectrometry, and infrared (IR) spectroscopy, and the solid-state structures were established by single-crystal X-ray diffraction analysis.
引用
收藏
页码:2086 / 2096
页数:11
相关论文
共 50 条
  • [41] CCD PHOTOMETRY FOR 6 METAL-RICH GALACTIC GLOBULAR-CLUSTERS
    SARAJEDINI, A
    NORRIS, JE
    ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1994, 93 (01): : 161 - &
  • [42] A photometric survey for variable stars in twelve metal-rich globular clusters
    Layden, AC
    Bowes, BT
    Ritter, LA
    Welch, DL
    Webb, TMA
    IMPACT OF LARGE-SCALE SURVEYS ON PULSATING STAR RESEARCH, 2000, 203 : 264 - 264
  • [43] On the production of bright RR Lyrae variables in metal-rich globular clusters
    Sweigart, AV
    Catelan, M
    HALF CENTURY OF STELLAR PULSATION INTERPRETATIONS: A TRIBUTE TO ARTHUR N. COX, 1998, 135 : 39 - 40
  • [44] TIO BAND STRENGTHS IN METAL-RICH GLOBULAR CLUSTERS .2.
    MOULD, J
    STUTMAN, D
    MCELROY, D
    ASTROPHYSICAL JOURNAL, 1979, 228 (02): : 423 - 429
  • [45] Metal-rich Trailing Outflows Uplifted by AGN Bubbles in Galaxy Clusters
    Duan, Xiaodong
    Guo, Fulai
    ASTROPHYSICAL JOURNAL, 2018, 861 (02):
  • [46] THE METAL ABUNDANCE OF METAL-RICH GLOBULAR-CLUSTERS .4. OXYGEN ABUNDANCES
    GRATTON, RG
    ASTRONOMY & ASTROPHYSICS, 1987, 177 (1-2) : 177 - 182
  • [47] Boron: Enabling Exciting Metal-Rich Structures and Magnetic Properties
    Scheifers, Jan P.
    Zhang, Yuemei
    Fokwa, Boniface P. T.
    ACCOUNTS OF CHEMICAL RESEARCH, 2017, 50 (09) : 2317 - 2325
  • [48] Metal-rich globular clusters in the galactic disk: new age determinations and the relation to halo clusters
    Salaris, M
    Weiss, A
    ASTRONOMY & ASTROPHYSICS, 1998, 335 (03) : 943 - 953
  • [49] SYNTHESIS OF METAL-RICH METALLABORANE CLUSTERS - EVIDENCE FOR A MECHANISM INVOLVING FRAGMENT CONDENSATION
    MENG, XS
    BANDYOPADHYAY, AK
    FEHLNER, TP
    GREVELS, FW
    JOURNAL OF ORGANOMETALLIC CHEMISTRY, 1990, 394 (1-3) : 15 - 27
  • [50] Two-step liquid drop model for binary, metal-rich clusters
    Despa, F
    PHYSICS LETTERS A, 2000, 276 (1-4) : 109 - 114