Recent Advances in Numerical Analysis.

1982 ◽  
Vol 38 (158) ◽  
pp. 654
Author(s):  
Carl de Boor ◽  
Gene H. Golub
Keyword(s):  
Numerical Analysis ◽  
Recent Advances

RECENT ADVANCES IN THE HIGHER SYSTEMATICS AND PHYLOGENETIC CONCEPTS IN ENTOMOLOGY

1973 ◽  
Vol 105 (9) ◽  
pp. 1251-1263 ◽  
Author(s):  
G. G. E. Scudder
Keyword(s):  
Numerical Analysis ◽  
Recent Work ◽  
Fossil Record ◽  
Recent Advances ◽  
Difference Of Opinion

AbstractThis paper reviews recent work on the higher systematics of insects and summarizes the various phylogenetic concepts advocated. It is evident that there is considerable difference of opinion. This is likely to prevail since the fossil record is inadequate. It is suggested that a numerical analysis of the insects at the Order level might be profitable.

Recent advances in the numerical analysis of heat pipes

1994 ◽  
Vol 14 (5) ◽  
pp. 480-491 ◽  
Author(s):  
A. Faghri
Keyword(s):  
Numerical Analysis ◽  
Heat Pipes ◽  
Recent Advances

Recent Advances in Applied Nonlinear Dynamics with Numerical Analysis

10.1142/8637 ◽  
2012 ◽  
Author(s):  
Changpin Li ◽  
Yujiang Wu ◽  
Ruisong Ye
Keyword(s):  
Nonlinear Dynamics ◽  
Numerical Analysis ◽  
Recent Advances

Recent Advances in High Dispersion Spectroscopy of Globular Cluster Stars

1988 ◽  
Vol 132 ◽  
pp. 525-530
Author(s):  
Raffaele G. Gratton
Keyword(s):  
Globular Cluster ◽  
Globular Clusters ◽  
High Dispersion ◽  
Photographic Material ◽  
Recent Advances ◽  
Metal Abundances ◽  
Ccd Detectors ◽  
Major Progress

The use CCD detectors has allowed a major progress in abundance derivations for globular cluster stars in the last years. Abundances deduced from high dispersion spectra now correlates well with other abundance indicators. I discuss some problems concerning the derivation of accurate metal abundances for globular clusters using high dispersion spectra from both the old photographic and the most recent CCD data. The discrepant low abundances found by Cohen (1980), from photographic material for M71 giants, are found to be due to the use of too high microturbulences.

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