... Soc. 376, 10331046 (2007) doi:10.1111/j.1365-2966.2007.11549.x Kinematics and stellar populations of the dwarf elliptical galaxy IC 3653 I. V. Chilingarian,1 1 2 ,2,3 P. Prugniel, 2,4 O. K. Sil'chenko1 and V. L. Afanasiev 5 Sternberg Astronomical Institute of the Moscow State University, Universitetsky pr. ... Fitting the spectra with synthetic single stellar populations (SSP), we found an SSPequivalent age of 5 Gyr and nearly solar metallicity [Fe/H] =-0.06 dex. ... 2007 The Authors. ...
R And SiO maser. S And SN (NGC 224). W And SiO maser. Z And Outbursts, average cycle 8400d. Porb = 758.8d, it reveals Z And itself in photometry during the low state. A quasi-period, P1, Z And about 656d is present during the outbursts. The beat period Z And between Porb and P1, about 5500d, is also found in the Z And photometric data. RS And H2O maser. RT And Min II = 9.28. P varies, current elements are given. RU And P varies strongly. RX And Porb = 0.209893d. RY And OH, H2O maser. SS And P2 = 650d, P3 =
Contrib Mineral Petrol (2009) 157:573-592 DOI 10.1007/s00410-008-0353-6 OR IGINAL PAPER Diffusion of divalent cations in garnet : multi-couple experiments A. L. Perchuk Ж M. Burchard Ж H.-P. Schertl Ж W. V. Maresch Ж T. V. Gerya Ж H.-J. Bernhardt Ж O. Vidal ... A summary of garnet compositions studied so far in experimental runs and the diffusivity data obtained for the major divalent cations is given in Table 1 and Fig. ... The profile mainly depends on the concentration of the host garnet. ...
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MODEL 1 ATOM 1 N MET 1 -10.162 -1.457 -.382 1.00 44.00 ATOM 2 CA MET 1 -9.634 -2.815 -.212 1.00 33.86 ATOM 3 C MET 1 -10.611 -3.853 -.756 1.00 37.66 ATOM 4 O MET 1 -11.833 -3.761 -.691 1.00 33.64 ATOM 5 CB MET 1 -9.307 -3.125 1.256 1.00 39.57 ATOM 6 CG MET 1 -10.446 -3.695 2.086 1.00 44.69 ATOM 7 SD MET 1 -10.071 -3.835 3.853 1.00 68.62 ATOM 8 CE MET 1 -10.944 -2.403 4.474 1.00 62.89 ATOM 9 N GLN 2 -10.047 -4.908 -1.344 1.00 30.80 ATOM 10 CA GLN 2 -10.851 -5.947 -1.969 1.00 29.90 ATOM 11 C GLN 2 -11.554
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