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Single crystals of the MgZn2Ce alloy (magnesium dizinc cerium) were synthesized by a two-step method which couples the thermal treatment of pressed pellets of the pure elements with subsequent arc melting. The compound crystallizes in a Heusler-type (MnCu2Al) structure in the space group Fm\overline{3}m, with one Zn site (site symmetry \overline{4}3m), one Ce and one Mg site (both with m\overline{3}m site symmetry). All inter­atomic distances indicate metallic type bonding.

Supporting information

cif

Crystallographic Information File (CIF) https://doi.org/10.1107/S1600536807028899/wm2125sup1.cif
Contains datablocks global, I

hkl

Structure factor file (CIF format) https://doi.org/10.1107/S1600536807028899/wm2125Isup2.hkl
Contains datablock I

Key indicators

  • Single-crystal X-ray study
  • T = 295 K
  • Mean [sigma](e-Zn) = 0.000 Å
  • R factor = 0.016
  • wR factor = 0.045
  • Data-to-parameter ratio = 11.0

checkCIF/PLATON results

No syntax errors found



Alert level C PLAT041_ALERT_1_C Calc. and Rep. SumFormula Strings Differ .... ? PLAT045_ALERT_1_C Calculated and Reported Z Differ by ............ 0.50 Ratio PLAT790_ALERT_4_C Centre of Gravity not Within Unit Cell: Resd. # 1 Ce2 Zn4
Alert level G REFLT03_ALERT_4_G Please check that the estimate of the number of Friedel pairs is correct. If it is not, please give the correct count in the _publ_section_exptl_refinement section of the submitted CIF. From the CIF: _diffrn_reflns_theta_max 32.96 From the CIF: _reflns_number_total 55 Count of symmetry unique reflns 1 Completeness (_total/calc) 5500.00% TEST3: Check Friedels for noncentro structure Estimate of Friedel pairs measured 54 Fraction of Friedel pairs measured 54.000 Are heavy atom types Z>Si present yes
0 ALERT level A = In general: serious problem 0 ALERT level B = Potentially serious problem 3 ALERT level C = Check and explain 1 ALERT level G = General alerts; check 2 ALERT type 1 CIF construction/syntax error, inconsistent or missing data 0 ALERT type 2 Indicator that the structure model may be wrong or deficient 0 ALERT type 3 Indicator that the structure quality may be low 2 ALERT type 4 Improvement, methodology, query or suggestion 0 ALERT type 5 Informative message, check

Comment top

Rare-earth transition metal intermetallics are intensively studied due to their useful physical properties. Mg-containing alloys tend to be particularly effective because of their high hydrogen uptake capacity at low density and cost. Among RE–T–Mg alloys (RE = rare earth, T = 3d transition metal), the most studied are Ni-containing alloys. Ternary phases with a 1:9:2 stoichiometry were studied by Kadir et al. (1997) and Solokha et al. (2006). Hydrogen uptake capacities of RENi4Mg (RE = Y, La, Nd) compounds with the MgCu4Sn structure type were determined by Aono et al. (2000) and Guénée et al. (2003). The crystal structure, chemical bonding and physical properties of RE2{Cu,Ni,Pd}2Mg ternaries with the Mo2FeB2 structure type were investigated by Lukachuk & Pöttgen (2003). It was shown that the Heusler-type alloy LaNi2Mg adsorbs H2 under formation of the quaternary metal hydride LaMg2NiH7 (Renaudin et al., 2003). Detailed investigations of fundamental properties of La–Ni–Mg (De Negri et al., 2005) and La–Cu–Mg (De Negri et al., 2006) phases at 673 K have indicated a great number of novel ternary phases in these systems. Recently, Solokha et al. (2007) studied the crystal structure of the novel phase Tb2Ni2Mg3 which does not form with the ligher rare earth metals.

The accurate determination of the crystal structure of new intermetallics is the basic requirement for a more detailed understanding of their properties. Here, we report the crystal structure of the ternary compound MgZn2Ce (I) based on single-crystal X-ray diffraction data.

The title compound (I) belongs to the Heusler-type alloys (MnCu2Al structure), with the Al site [Wyckoff position 4a] now occupied by Ce atoms, and the Mn [4b] and Cu [8c] atoms replaced by Mg and Zn atoms, respectively. The unit cell projection of (I) is shown in Fig. 1. The first coordination spheres of all atoms are the same as for the cubic close packed (c.c.p.) structures, viz. a rhombododecahedron with a coordination number of 14. The interatomic distances are in good correlation with the sums of the atomic radii (Emsley, 1991) and indicate a typical metallic type bonding, with the shortest Ce–Zn distance of 3.04659 (17) Å which is 96.2% of the sum of the atomic radii.

Related literature top

Other ternary alloys in the system RE–T–Mg (RE = rare earth metal and T = transition metal) and their properties have been studied by: Kadir et al. (1997); Solokha et al. (2006, 2007); Aono et al. (2000); Guénée et al. (2003); Lukachuk & Pöttgen (2003); Renaudin et al. (2003); De Negri et al., (2005, 2007). Tests for centrosymmetric or non-centrosymmetric space groups were performed using the WinGX program by Farrugia (1999), following the advice of Marsh (1995). Atomic radii for the elements were taken from Emsley (1991) and the atomic coordinates were standardized using the STRUCTURE-TIDY program by Gelato & Parthé (1987).

Experimental top

With the purpose to avoid losses of magnesium and zinc due to their low vapour pressure at higher temperatures, the alloys were prepared in two steps. In a first step the powders of the pure elements (stoichiometry Mg:Zn:Ce = 1:2:1) were pressed into a pellet and enclosed in evacuated silica ampoules (pressure inside 10-5 to 10 -6 Pa), which were then placed in a resistance furnace with a thermocouple controller. The heating process was carried out in consecutive order. Firstly, the ampoule was heated at 673 K for four d, then the temperature was increased to 873 K and held for two d. The ampoules were then heated up to 1073 K (held for four h and slowly cooled down to room temperature). In a second step, the pellets were remelted in an arc furnace. The samples were stable against air and moisture, irrespective whether they were in the form of compact pellets or as fine-grained powders. Wavelength dispersive spectrometry and electron probe microanalysis (CAMECA SX100 analyser) were used to control the number of phases and their content in the samples. An average result of the microprobe analysis for the title compound is 25.6%at Ce, 25.8%at Zn and 48.6%at Mg which compares well with the composition obtained from the structure refinement. Irregularly shaped single crystals, exhibiting metallic luster, were isolated by mechanical fragmentation from the alloys.

Refinement top

Systematic absences indicated possible space groups F23 (#196), Fm3 (#202), F432 (#209), F43m (#216), and centrosymmetric Fm3m (#225). The statistical test of the distribution of the E values (Farrugia, 1999) suggested that the structure is centrosymmetric with a probability of 55.1%. However, following the advice of Marsh (1995) the structure solution and refinement were also performed in non-centrosymmetric space groups. The results clearly indicated that compound (I) crystallizes in the centrosymmetric space group Fm3m. The s.o.f. parameters were refined for this structure in order to check the deviations from the ideal stoichiometry, but no significant deviations were found. Therefore in the final refinement cycles the full occupancy parameters were retained and all atoms were refined with anisotropic displacement parameters. Finally, the atomic coordinates were standardized using the STRUCTURE-TIDY program (Gelato & Parthé, 1987). The final difference Fourier syntheses revealed no significant residual peaks - the highest maximum electron density is 0.95 Å from Ce and the deepest hole is 1.32 Å from Zn.

Structure description top

Rare-earth transition metal intermetallics are intensively studied due to their useful physical properties. Mg-containing alloys tend to be particularly effective because of their high hydrogen uptake capacity at low density and cost. Among RE–T–Mg alloys (RE = rare earth, T = 3d transition metal), the most studied are Ni-containing alloys. Ternary phases with a 1:9:2 stoichiometry were studied by Kadir et al. (1997) and Solokha et al. (2006). Hydrogen uptake capacities of RENi4Mg (RE = Y, La, Nd) compounds with the MgCu4Sn structure type were determined by Aono et al. (2000) and Guénée et al. (2003). The crystal structure, chemical bonding and physical properties of RE2{Cu,Ni,Pd}2Mg ternaries with the Mo2FeB2 structure type were investigated by Lukachuk & Pöttgen (2003). It was shown that the Heusler-type alloy LaNi2Mg adsorbs H2 under formation of the quaternary metal hydride LaMg2NiH7 (Renaudin et al., 2003). Detailed investigations of fundamental properties of La–Ni–Mg (De Negri et al., 2005) and La–Cu–Mg (De Negri et al., 2006) phases at 673 K have indicated a great number of novel ternary phases in these systems. Recently, Solokha et al. (2007) studied the crystal structure of the novel phase Tb2Ni2Mg3 which does not form with the ligher rare earth metals.

The accurate determination of the crystal structure of new intermetallics is the basic requirement for a more detailed understanding of their properties. Here, we report the crystal structure of the ternary compound MgZn2Ce (I) based on single-crystal X-ray diffraction data.

The title compound (I) belongs to the Heusler-type alloys (MnCu2Al structure), with the Al site [Wyckoff position 4a] now occupied by Ce atoms, and the Mn [4b] and Cu [8c] atoms replaced by Mg and Zn atoms, respectively. The unit cell projection of (I) is shown in Fig. 1. The first coordination spheres of all atoms are the same as for the cubic close packed (c.c.p.) structures, viz. a rhombododecahedron with a coordination number of 14. The interatomic distances are in good correlation with the sums of the atomic radii (Emsley, 1991) and indicate a typical metallic type bonding, with the shortest Ce–Zn distance of 3.04659 (17) Å which is 96.2% of the sum of the atomic radii.

Other ternary alloys in the system RE–T–Mg (RE = rare earth metal and T = transition metal) and their properties have been studied by: Kadir et al. (1997); Solokha et al. (2006, 2007); Aono et al. (2000); Guénée et al. (2003); Lukachuk & Pöttgen (2003); Renaudin et al. (2003); De Negri et al., (2005, 2007). Tests for centrosymmetric or non-centrosymmetric space groups were performed using the WinGX program by Farrugia (1999), following the advice of Marsh (1995). Atomic radii for the elements were taken from Emsley (1991) and the atomic coordinates were standardized using the STRUCTURE-TIDY program by Gelato & Parthé (1987).

Computing details top

Data collection: CrysAlis CCD (Oxford Diffraction, 2004); cell refinement: CrysAlis CCD; data reduction: CrysAlis RED (Oxford Diffraction, 2005); program(s) used to solve structure: SHELXS97 (Sheldrick, 1997); program(s) used to refine structure: SHELXL97 (Sheldrick, 1997); molecular graphics: DIAMOND (Brandenburg, 1999); software used to prepare material for publication: SHELXL97.

Figures top
[Figure 1] Fig. 1. Perspective view of the unit-cell projection of (I) on the (001) plane. Coordination polyhedra of Ce (a), Zn (b) and Mg (c) are shown.
Magnesium dizinc cerium top
Crystal data top
MgZn2CeDx = 5.629 Mg m3
Mr = 295.17Mo Kα radiation, λ = 0.71073 Å
Cubic, Fm3mCell parameters from 764 reflections
Hall symbol: -F 4 2 3θ = 5.0–33.0°
a = 7.0358 (4) ŵ = 26.40 mm1
V = 348.29 (3) Å3T = 295 K
Z = 4Irregular, metallic dark-grey
F(000) = 5200.10 × 0.08 × 0.06 mm
Data collection top
Oxford Diffraction Xcalibur CCD
diffractometer
55 independent reflections
Radiation source: fine-focus sealed tube55 reflections with I > 2σ(I)
Graphite monochromatorRint = 0.053
ω scansθmax = 33.0°, θmin = 5.0°
Absorption correction: analytical
(CrysAlis RED; Oxford Diffraction, 2005)
h = 107
Tmin = 0.11, Tmax = 0.198k = 1010
764 measured reflectionsl = 910
Refinement top
Refinement on F2Primary atom site location: structure-invariant direct methods
Least-squares matrix: fullSecondary atom site location: difference Fourier map
R[F2 > 2σ(F2)] = 0.016 w = 1/[σ2(Fo2) + (0.0117P)2 + 19.6603P]
where P = (Fo2 + 2Fc2)/3
wR(F2) = 0.045(Δ/σ)max < 0.001
S = 1.01Δρmax = 0.95 e Å3
55 reflectionsΔρmin = 1.32 e Å3
5 parametersExtinction correction: SHELXL97 (Sheldrick, 1997), Fc*=kFc[1+0.001xFc2λ3/sin(2θ)]-1/4
0 restraintsExtinction coefficient: 0.0038 (5)
Crystal data top
MgZn2CeZ = 4
Mr = 295.17Mo Kα radiation
Cubic, Fm3mµ = 26.40 mm1
a = 7.0358 (4) ÅT = 295 K
V = 348.29 (3) Å30.10 × 0.08 × 0.06 mm
Data collection top
Oxford Diffraction Xcalibur CCD
diffractometer
55 independent reflections
Absorption correction: analytical
(CrysAlis RED; Oxford Diffraction, 2005)
55 reflections with I > 2σ(I)
Tmin = 0.11, Tmax = 0.198Rint = 0.053
764 measured reflections
Refinement top
R[F2 > 2σ(F2)] = 0.0160 restraints
wR(F2) = 0.045 w = 1/[σ2(Fo2) + (0.0117P)2 + 19.6603P]
where P = (Fo2 + 2Fc2)/3
S = 1.01Δρmax = 0.95 e Å3
55 reflectionsΔρmin = 1.32 e Å3
5 parameters
Special details top

Geometry. All e.s.d.'s (except the e.s.d. in the dihedral angle between two l.s. planes) are estimated using the full covariance matrix. The cell e.s.d.'s are taken into account individually in the estimation of e.s.d.'s in distances, angles and torsion angles; correlations between e.s.d.'s in cell parameters are only used when they are defined by crystal symmetry. An approximate (isotropic) treatment of cell e.s.d.'s is used for estimating e.s.d.'s involving l.s. planes.

Refinement. Refinement of F2 against ALL reflections. The weighted R-factor wR and goodness of fit S are based on F2, conventional R-factors R are based on F, with F set to zero for negative F2. The threshold expression of F2 > σ(F2) is used only for calculating R-factors(gt) etc. and is not relevant to the choice of reflections for refinement. R-factors based on F2 are statistically about twice as large as those based on F, and R- factors based on ALL data will be even larger.

Fractional atomic coordinates and isotropic or equivalent isotropic displacement parameters (Å2) top
xyzUiso*/Ueq
Ce0.00000.00000.00000.0098 (4)
Zn0.25000.25000.25000.0153 (4)
Mg0.50000.50000.50000.0112 (11)
Atomic displacement parameters (Å2) top
U11U22U33U12U13U23
Ce0.0098 (4)0.0098 (4)0.0098 (4)0.0000.0000.000
Zn0.0153 (4)0.0153 (4)0.0153 (4)0.0000.0000.000
Mg0.0112 (11)0.0112 (11)0.0112 (11)0.0000.0000.000
Geometric parameters (Å, º) top
Ce—Zni3.0466 (2)Zn—Cexi3.0466 (2)
Ce—Zn3.0466 (2)Zn—Cexii3.0466 (2)
Ce—Znii3.0466 (2)Zn—Mgv3.0466 (2)
Ce—Zniii3.0466 (2)Zn—Mgiii3.0466 (2)
Ce—Zniv3.0466 (2)Mg—Znxiii3.0466 (2)
Ce—Znv3.0466 (2)Mg—Znxiv3.0466 (2)
Ce—Znvi3.0466 (2)Mg—Znxv3.0466 (2)
Ce—Znvii3.0466 (2)Mg—Znxvi3.0466 (2)
Ce—Mgiv3.5179 (2)Mg—Znxii3.0466 (2)
Ce—Mgviii3.5179 (2)Mg—Znxi3.0466 (2)
Ce—Mgv3.5179 (2)Mg—Znx3.0466 (2)
Ce—Mgix3.5179 (2)Mg—Cexvii3.5179 (2)
Zn—Mg3.0466 (2)Mg—Cexviii3.5179 (2)
Zn—Mgiv3.0466 (2)Mg—Cexii3.5179 (2)
Zn—Cex3.0466 (2)Mg—Cex3.5179 (2)
Zni—Ce—Zn180.0Cexi—Zn—Cexii109.5
Zni—Ce—Znii109.5Mg—Zn—Mgv109.5
Zn—Ce—Znii70.5Ce—Zn—Mgv70.5
Zni—Ce—Zniii70.5Mgiv—Zn—Mgv109.5
Zn—Ce—Zniii109.5Cex—Zn—Mgv180.0
Znii—Ce—Zniii70.5Cexi—Zn—Mgv70.5
Zni—Ce—Zniv70.5Cexii—Zn—Mgv70.5
Zn—Ce—Zniv109.5Mg—Zn—Mgiii109.5
Znii—Ce—Zniv180.0Ce—Zn—Mgiii70.5
Zniii—Ce—Zniv109.5Mgiv—Zn—Mgiii109.5
Zni—Ce—Znv70.5Cex—Zn—Mgiii70.5
Zn—Ce—Znv109.5Cexi—Zn—Mgiii180.0
Znii—Ce—Znv70.5Cexii—Zn—Mgiii70.5
Zniii—Ce—Znv109.5Mgv—Zn—Mgiii109.5
Zniv—Ce—Znv109.5Znxiii—Mg—Zn180.0
Zni—Ce—Znvi109.5Znxiii—Mg—Znxiv109.5
Zn—Ce—Znvi70.5Zn—Mg—Znxiv70.5
Znii—Ce—Znvi109.5Znxiii—Mg—Znxv109.5
Zniii—Ce—Znvi70.5Zn—Mg—Znxv70.5
Zniv—Ce—Znvi70.5Znxiv—Mg—Znxv109.5
Znv—Ce—Znvi180.0Znxiii—Mg—Znxvi109.5
Zni—Ce—Znvii109.5Zn—Mg—Znxvi70.5
Zn—Ce—Znvii70.5Znxiv—Mg—Znxvi109.5
Znii—Ce—Znvii109.5Znxv—Mg—Znxvi109.5
Zniii—Ce—Znvii180.0Znxiii—Mg—Znxii70.5
Zniv—Ce—Znvii70.5Zn—Mg—Znxii109.5
Znv—Ce—Znvii70.5Znxiv—Mg—Znxii180.0
Znvi—Ce—Znvii109.5Znxv—Mg—Znxii70.5
Zni—Ce—Mgiv125.3Znxvi—Mg—Znxii70.5
Zn—Ce—Mgiv54.7Znxiii—Mg—Znxi70.5
Znii—Ce—Mgiv125.3Zn—Mg—Znxi109.5
Zniii—Ce—Mgiv125.3Znxiv—Mg—Znxi70.5
Zniv—Ce—Mgiv54.7Znxv—Mg—Znxi180.0
Znv—Ce—Mgiv125.3Znxvi—Mg—Znxi70.5
Znvi—Ce—Mgiv54.7Znxii—Mg—Znxi109.5
Znvii—Ce—Mgiv54.7Znxiii—Mg—Znx70.5
Zni—Ce—Mgviii54.7Zn—Mg—Znx109.5
Zn—Ce—Mgviii125.3Znxiv—Mg—Znx70.5
Znii—Ce—Mgviii125.3Znxv—Mg—Znx70.5
Zniii—Ce—Mgviii54.7Znxvi—Mg—Znx180.0
Zniv—Ce—Mgviii54.7Znxii—Mg—Znx109.5
Znv—Ce—Mgviii125.3Znxi—Mg—Znx109.5
Znvi—Ce—Mgviii54.7Znxiii—Mg—Cexvii54.7
Znvii—Ce—Mgviii125.3Zn—Mg—Cexvii125.3
Mgiv—Ce—Mgviii90.0Znxiv—Mg—Cexvii125.3
Zni—Ce—Mgv125.3Znxv—Mg—Cexvii125.3
Zn—Ce—Mgv54.7Znxvi—Mg—Cexvii54.7
Znii—Ce—Mgv54.7Znxii—Mg—Cexvii54.7
Zniii—Ce—Mgv125.3Znxi—Mg—Cexvii54.7
Zniv—Ce—Mgv125.3Znx—Mg—Cexvii125.3
Znv—Ce—Mgv54.7Znxiii—Mg—Cexviii54.7
Znvi—Ce—Mgv125.3Zn—Mg—Cexviii125.3
Znvii—Ce—Mgv54.7Znxiv—Mg—Cexviii54.7
Mgiv—Ce—Mgv90.0Znxv—Mg—Cexviii125.3
Mgviii—Ce—Mgv180.0Znxvi—Mg—Cexviii125.3
Zni—Ce—Mgix54.7Znxii—Mg—Cexviii125.3
Zn—Ce—Mgix125.3Znxi—Mg—Cexviii54.7
Znii—Ce—Mgix125.3Znx—Mg—Cexviii54.7
Zniii—Ce—Mgix125.3Cexvii—Mg—Cexviii90.0
Zniv—Ce—Mgix54.7Znxiii—Mg—Cexii125.3
Znv—Ce—Mgix54.7Zn—Mg—Cexii54.7
Znvi—Ce—Mgix125.3Znxiv—Mg—Cexii125.3
Znvii—Ce—Mgix54.7Znxv—Mg—Cexii54.7
Mgiv—Ce—Mgix90.0Znxvi—Mg—Cexii54.7
Mgviii—Ce—Mgix90.0Znxii—Mg—Cexii54.7
Mgv—Ce—Mgix90.0Znxi—Mg—Cexii125.3
Mg—Zn—Ce180.0Znx—Mg—Cexii125.3
Mg—Zn—Mgiv109.5Cexvii—Mg—Cexii90.0
Ce—Zn—Mgiv70.5Cexviii—Mg—Cexii180.0
Mg—Zn—Cex70.5Znxiii—Mg—Cex125.3
Ce—Zn—Cex109.5Zn—Mg—Cex54.7
Mgiv—Zn—Cex70.5Znxiv—Mg—Cex54.7
Mg—Zn—Cexi70.5Znxv—Mg—Cex54.7
Ce—Zn—Cexi109.5Znxvi—Mg—Cex125.3
Mgiv—Zn—Cexi70.5Znxii—Mg—Cex125.3
Cex—Zn—Cexi109.5Znxi—Mg—Cex125.3
Mg—Zn—Cexii70.5Znx—Mg—Cex54.7
Ce—Zn—Cexii109.5Cexvii—Mg—Cex180.0
Mgiv—Zn—Cexii180.0Cexviii—Mg—Cex90.0
Cex—Zn—Cexii109.5Cexii—Mg—Cex90.0
Symmetry codes: (i) x, y, z; (ii) x+1/2, y+1/2, z; (iii) x1/2, y, z1/2; (iv) x1/2, y1/2, z; (v) x, y1/2, z1/2; (vi) x, y+1/2, z+1/2; (vii) x+1/2, y, z+1/2; (viii) x1, y1/2, z1/2; (ix) x1/2, y1, z1/2; (x) x, y+1/2, z+1/2; (xi) x+1/2, y, z+1/2; (xii) x+1/2, y+1/2, z; (xiii) x+1, y+1, z+1; (xiv) x+1/2, y+1/2, z+1; (xv) x+1/2, y+1, z+1/2; (xvi) x+1, y+1/2, z+1/2; (xvii) x+1, y+1/2, z+1/2; (xviii) x+1/2, y+1/2, z+1.

Experimental details

Crystal data
Chemical formulaMgZn2Ce
Mr295.17
Crystal system, space groupCubic, Fm3m
Temperature (K)295
a (Å)7.0358 (4)
V3)348.29 (3)
Z4
Radiation typeMo Kα
µ (mm1)26.40
Crystal size (mm)0.10 × 0.08 × 0.06
Data collection
DiffractometerOxford Diffraction Xcalibur CCD
Absorption correctionAnalytical
(CrysAlis RED; Oxford Diffraction, 2005)
Tmin, Tmax0.11, 0.198
No. of measured, independent and
observed [I > 2σ(I)] reflections
764, 55, 55
Rint0.053
(sin θ/λ)max1)0.765
Refinement
R[F2 > 2σ(F2)], wR(F2), S 0.016, 0.045, 1.01
No. of reflections55
No. of parameters5
w = 1/[σ2(Fo2) + (0.0117P)2 + 19.6603P]
where P = (Fo2 + 2Fc2)/3
Δρmax, Δρmin (e Å3)0.95, 1.32

Computer programs: CrysAlis CCD (Oxford Diffraction, 2004), CrysAlis CCD, CrysAlis RED (Oxford Diffraction, 2005), SHELXS97 (Sheldrick, 1997), SHELXL97 (Sheldrick, 1997), DIAMOND (Brandenburg, 1999), SHELXL97.

Selected bond lengths (Å) top
Ce—Zn3.0466 (2)Zn—Mg3.0466 (2)
Ce—Mgi3.5179 (2)
Symmetry code: (i) x1, y1/2, z1/2.
 

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