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Now showing items 7131-7140 of 7165
Making Sense of Information- A New Role for the Marketing Researcher
(2000)
The value of today's business is measured increasingly in terms of what it knows, rather than what it owns. Even so, whilst knowledge exists in most organisations it is regularly difficult to access. This paper addresses ...
Learning how to do things with imitation
(AAAI, 2000)
In this paper we discuss how agents can learn to do things by imitating other agents. Especially we look at how the use of different metrics and sub-goal granularity can affect the imitation results. We use a computer model ...
On authority and revocation : Climacus as humorist
(Rodopi, 2000)
The morphology of the Magellanic Clouds revealed by stars of different age: results from the DENIS survey
(2000)
The spatial distribution of sources populating different regions of the colour–magnitude diagram (I −J,I) extracted from the DENIS catalogue towards the Mag- ellanic Clouds (DCMC – Cioni et al. 2000) reveal signifi- cantly ...
Abundances in very metal-poor stars
(Institut d'Astrophysique et de Geophysique, 2000)
Metal-poor stars provide information on the characteristics and chemical evolution of the halo population of the Galaxy, the first epoch of star formation and Galaxy formation (not just locally but with relevance to ...
Retirement, Household Income, and Economic Vulnerability of Older Groups
(University of Hertfordshire, 2000)
This paper examines retirement behaviour and household income for older persons in Chile. It pays close attention to the sources of household income, income inequalities, and the economic vulnerability of older persons. ...
Primordial Lithium and Big Bang Nucleosynthesis
(2000)
Recent determinations of the abundance of the light-element Li in very metal-poor stars show that its intrinsic dispersion is essentially zero and that the random error in the estimated mean Li abundance is negligible. ...
VLBI observations of two single dMe stars: spatial resolution and astrometry
(2000)
We report on 3.6 cm VLA and VLBA observations of YZ CMi and AD Leo, two nearby dMe stars. We resolve YZ CMi and can fit a circular symmetrical gaussian component of FWHP of 0.98 0.2 mas, corresponding to an extent of the ...