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7篇 您的检索式:作者名="Binil"
    题名 作者 年代 出处 被引量
1Mechanical evaluation of porous titanium (Ti6AI4V) structures with electron beam melting(EBM)显示文摘Jayanthi Parthasarathy Starlya Binil Shivakumar Raman 2010Joumal of the Mechanical Behavior of Biomedical Materials2010,3,3:1
2A design for the additive manufacture of functionally graded porous structures with tailored mechanical properties for biomedical applications显示文摘Jayanthi Parthasarathy Binil Starly Shivakumar Raman 2011Journal of Manufacturing Processes2011,,2:1
3Alginate based 3D hydrogels as an in vitro co-culture model platform for the toxicity screening of new chemical entities 显示文摘Lan Shih-Feng and Starly Binil 2011Toxicology and Applied Pharmacology2011,256,1:1
4In vitro antioxidant activities of the methanol extract and its different solvent fractions obtained from the fruit pericarp of Terminalia bellerica 显示文摘Nampoothiri S V Binil Raj S S Prathapan A 2011Nat Prod Res2011,25,3:1
5Direct slicing of STEP based NURBS models for layered manufacturing 显示文摘Binil Stady Alan Lau 2005Computer-Aided Design (S0010-4485)2005,37,1:1
6Winding sense of galaxies around the local supercluster显示文摘We present an analysis of the winding sense(S and Z-shapes) of 1 621 field galaxies that have radial velocity between 3 000 km s-1 and 5 000 km s-1.The preferred alignments of S-and Z-shaped galaxies are studied using chi-square,autocorrelation and Fourier series tests.We classify all the galaxies into 32 subsamples and notice a good agreement between the position angle(PA) distribution of the S-and Zshaped galaxies.The homogeneous distribution of the S-and Z-shaped galaxies is more noticeable for the late-type spirals(Sc,Scd,Sd and Sm) than for the early-types(Sa,Sab,Sb and Sbc) .A significant dominance of S-mode galaxies is apparent in the barred spirals.A random alignment is evident in the PA-distribution of Z-and S-mode spirals.In addition,a homogeneous distribution of the S-and Z-shaped galaxies is found to be invariant under global expansion.The PA-distribution of the total S-mode galaxies is found to be random,whereas a preferred alignment is clear for all the Zmode galaxies.It is found that the galactic planes of Z-mode galaxies tend to lie in the equatorial plane.Binil Aryal 2011Research in Astronomy and Astrophysics2011,11,3:0
7Preferred alignments of angular momentum vectors of galaxies in six dynamically unstable Abell clusters显示文摘A spatial orientation of angular momentum vectors of galaxies in six dynamically unstable Abell clusters(S1171, S0001, A1035, A1373, A1474 and A4053) is studied. For this, twodimensional observed parameters(e.g., positions, diameters and position angles) are converted into three-dimensional(3D) rotation axes of the galaxy using the ‘position angle-inclination' method. The expected isotropic distribution curves for angular momentum vectors are obtained by performing random simulations. The observed and expected distributions are compared using several statistical tests.No preferred alignments of angular momentum vectors of galaxies are noticed in all six dynamically unstable clusters, supporting the hierarchy model of galaxy formation. These clusters have a larger value of velocity dispersion. However, local effects are noticed in the clusters that have substructures in the1D-3D number density maps.Shiv N.Yadav Binil Aryal Walter Saurer 2017Research in Astronomy and Astrophysics2017,17,7:0
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