Degraded divinity? Sacred monstrosity? Gérard Depardieu and the abject star body

Screen ◽  
2015 ◽  
Vol 56 (3) ◽  
pp. 319-334
Author(s):  
Sue Harris
Keyword(s):  
1949 ◽  
Vol 1 (1) ◽  
pp. 78-87 ◽  
Author(s):  
K. Mahler

In this note, I shall establish necessary and sufficient conditions for the existence of critical lattices of an arbitrary point set, and I shall construct a non-trivial example of a point set without any critical lattice. In a previous paper, I proved that every star body of the finite type possesses at least one critical lattice.


2017 ◽  
Vol 25 (1) ◽  
pp. 5-11 ◽  
Author(s):  
Werner Georg Nowak

Abstract In a classic paper [14], W.G. Spohn established the to-date sharpest estimates from below for the simultaneous Diophantine approximation constants for three and more real numbers. As a by-result of his method which used Blichfeldt’s Theorem and the calculus of variations, he derived a bound for the critical determinant of the star body|x1|(|x1|3 + |x2|3 + |x3|3 ≤ 1.In this little note, after a brief exposition of the basics of the geometry of numbers and its significance for Diophantine approximation, this latter result is improved and extended to the star body|x1|(|x1|3 + |x22 + x32)3/2≤ 1.


1998 ◽  
Author(s):  
John Sabean ◽  
Mark Lewis ◽  
David Mee ◽  
Allan Paull

2022 ◽  
Vol 5 (1) ◽  
Author(s):  
Ben Thuy ◽  
Mats E. Eriksson ◽  
Manfred Kutscher ◽  
Johan Lindgren ◽  
Lea D. Numberger-Thuy ◽  
...  

AbstractPivotal anatomical innovations often seem to appear by chance when viewed through the lens of the fossil record. As a consequence, specific driving forces behind the origination of major organismal clades generally remain speculative. Here, we present a rare exception to this axiom by constraining the appearance of a diverse animal group (the living Ophiuroidea) to a single speciation event rather than hypothetical ancestors. Fossils belonging to a new pair of temporally consecutive species of brittle stars (Ophiopetagno paicei gen. et sp. nov. and Muldaster haakei gen. et sp. nov.) from the Silurian (444–419 Mya) of Sweden reveal a process of miniaturization that temporally coincides with a global extinction and environmental perturbation known as the Mulde Event. The reduction in size from O. paicei to M. haakei forced a structural simplification of the ophiuroid skeleton through ontogenetic retention of juvenile traits, thereby generating the modern brittle star bauplan.


2021 ◽  
pp. 19-50
Author(s):  
Lisa Stead

The chapter explores the archival record of Vivien Leigh’s stage and screen craft. It considers how the archive illuminates her struggle to position her performative talent and craft in the “right” way relative to her status as glamourous star body. The chapter interrogates material in her archive at the V&A, her papers at the British Library, and connected archives of those performers and directors with whom she worked. Key case studies include her written correspondence with Laurence Olivier during the filming of Gone with the Wind, which illuminates her approach to male mentorship more broadly across her career. The chapter also focusses on two key aspects of her stage and screen craft often singled out for criticism in the reception of her performances: her voice and physical stamina.


1959 ◽  
Vol 11 ◽  
pp. 256-261 ◽  
Author(s):  
A. C. Woods

We select a Cartesian co-ordinate system in ndimensional Euclidean space Rn with origin 0 and employ the usual pointvector notation.By a lattice Λ in Rn we mean the set of all rational integral combinations of n linearly independent points X1, X2, … , Xn of Rn. The points X1 X2, … , Xn are said to form a basis of Λ. Let {X1, X2, … , Xn) denote the determinant formed when the co-ordinates of Xi are taken in order as the ith row of the determinant for i = 1,2, … , n. The absolute value of this determinant is called the determinant d(Λ) of Λ. It is well known that d(Λ) is independent of the particular basis one takes for Λ.A star body in Rn is a closed set of points K such that if X ∈ K then every point of the form tX where — 1 < t < 1 is an inner point of K.


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