Predicting the peculiar velocities of nearby PSCz galaxies using the Least Action Principle

Monthly Notices of the Royal Astronomical Society

Volumn 322, Issue 1, 2001, Pages 121-130

  Sharpe, J ^a   Rowan Robinson, M ^a   Canavezes, A ^a   Saunders, W ^b   Branchini, E ^c   Efstathiou, G ^d   Frenk, C ^c   Keeble, O ^a   McMahon, R G ^d   Maddox, S ^d   Oliver, S J ^a   Sutherland, W ^e   Tadros, H ^e,f   White, S D M ^g  

^a IMPERIAL COLLEGE LONDON   (United Kingdom)

^b UNIVERSITY OF EDINBURGH   (United Kingdom)

^c DURHAM UNIVERSITY   (United Kingdom)

^d UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^e UNIVERSITY OF OXFORD   (United Kingdom)

^f UNIVERSITY OF SUSSEX   (United Kingdom)

^g MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

Author keywords

Dark matter; Distance scale; Galaxies: distances and redshifts; Large scale structure of Universe; Methods: numerical

Indexed keywords

ASTROPHYSICS; FORECASTING; NUMERICAL METHODS; STARS; VELOCITY;

CEPHEID DISTANCE; DARK MATTER; DISTANCE SCALE; GALAXIES DISTANCES AND REDSHIFTS; LARGE SCALE STRUCTURE OF UNIVERSE; LEAST-ACTION PRINCIPLES; LINEAR THEORY; METHOD: NUMERICAL; PECULIAR VELOCITIES; TIDAL EFFECTS;

GALAXIES;

EID: 18044404599     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2001.04123.x     Document Type: Article

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