Lynden-Bell

Lynden-Bell R M and Rasaiah J C 1997 From hydrophobic to hydrophilic behavior a simulation study of solvation entropy and free energy of simple solutes J. Chem. Phys. 107 1981... 

Lynden-Bell R M and Harris R K 1969 Nuclear Magnetic Resonance Spectroscopy (London Nelson) pp 81-3... 

Lynden-Bell R M, van Duijneveldt J S and Frenkel D 1993 Free-energy changes on freezing and melting ductile metals Mol. Phys. 80 801-14... 

In order to describe the incoherent exchange, in the pulse collision model [Lynden-Bell 1964 Johnson 1967 Stunzes and Benderskii 1971] an effective exchange term, whose real part is... 

W. Robert Carper, Andreas Ddlle, Christof G. Hanke, Chris Hardacre, Axel Leuchter, Ruth M. Lynden-Bell, Zhizhong Meng, Gunter Palmer, and Joachim Richter... 

Lynden-Bell R. M. The effect of molecular reorientation on the line-shapes of degenerate vibrations in infra-red and Raman spectra of liquids, Mol. Phys. 31, 1653-62 (1976). 

Madden P. A., Lynden-Bell R. M. Theory of vibrational line-widths,... 

Lynden-Bell R. M. In Molecular Liquids Dynamics and Interactions, eds. A. J. Barnes, W. J. Orville-Thomas, J. Yarwood. (Reidel, Dordrecht) (1984). 

LD Gelb and RM Lynden-Bell, Chem. Phys. Lett. 211 (1993) 328. 

R. M. Lynden-Bell, Prog. Sucl. Magn Reson. Spectrosc., 2 (1967) 163-204. 

Lozovoi AY, Alavi A, Kohanoff J, Lynden-Bell RM. 2001. Ah initio simulation of charged slabs at constant chemical potential. J Chem Phys 115 1661-1669. 

Fig. 3.39. Correlations between UV excess and stellar orbital eccentricity and velocity at right angles to the plane of the Milky Way. Adapted from Eggen, Lynden-Bell and Sandage (1962).

D. Lynden-Bell and G. Gilmore (eds.), Baryonic Dark Matter, Kluwer, Dordrecht, 1990, and in Sarkar (1996). 

Fig. 8.25. Theoretical abundance distribution functions according to Lynden-Bell s Best Accretion Model for different values of M, after Pagel (1989b).

Alternative wind models assume a selective outflow of enriched material, either taking place at the time of star formation bursts in dwarf galaxies (Matteucci Tosi 1985) or taking place continuously from the hot component of the ISM which is also assumed to be metal-enriched (Vader 1987 Ferreras, Scannapieco Silk 2002). An analytical model by Lynden-Bell (1992) supposes that, of the return fraction 1 — a from a generation of stars, a fraction 1 — / escapes, leading via Eq. (7.34) to... 

The offsets of axes determine the characteristic mass Me that constrains supernova debris and the true yield y (p in the text). MB is the corresponding blue absolute magnitude (neglecting any dark halos). The trend along the linear branch of the curve is for metallicity to increase approximately as A/1/2. After Lynden-Bell (1992). 

O.J. Eggen, D. Lynden-Bell and Sandage assemble dynamical and chemical evidence for formation of the Galaxy by free-fall collapse. The issue is still debated. 

Lynden-Bell, D. 1973, in G. Contopulos, M. Henon D. Lynden-Bell, Dynamical Structure and Evolution of Stellar Systems, Geneva Geneva Observatory, p. 132. Lynden-Bell, D. 1975, Vistas in Astr., 19, 299. 

Lynden-Bell, D. 1992, in M. G. Edmunds R. J. Terlevich (eds.), Elements and the Cosmos, Cambridge Cambridge University Press, p. 270. 

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