Does the Professional Manager Blow the Whistle on Founding Families? New Evidence on the Dark Side of Family-Controlled Firm

2016 ◽  
Author(s):  
Hansoo Choi ◽  
Changmin Lee
PLoS ONE ◽  
2017 ◽  
Vol 12 (6) ◽  
pp. e0178652 ◽  
Author(s):  
Juliana Gabrielle Martins ◽  
Haroldo Neves de Paiva ◽  
Paula Cristina Pelli Paiva ◽  
Raquel Conceição Ferreira ◽  
Isabela Almeida Pordeus ◽  
...  

Sociology ◽  
2018 ◽  
Vol 53 (2) ◽  
pp. 401-421 ◽  
Author(s):  
Xianbi Huang ◽  
Mark Western ◽  
Yanjie Bian ◽  
Yaojun Li ◽  
Rochelle Côté ◽  
...  

The article draws on data from a national survey in Australia in 2014 to examine how social networks affect life satisfaction and happiness. Findings show that social network composition, social attachment, perceived social support and the volume of social resources are significantly positively associated with life satisfaction and happiness. Stress about social commitments, feeling restricted by social demands and being excluded by a social group are negatively associated with life satisfaction and happiness. These results indicate that social networks have both ‘bright side’ and ‘dark side’ effects on subjective wellbeing.


1978 ◽  
Vol 48 ◽  
pp. 31-35
Author(s):  
R. B. Hanson

Several outstanding problems affecting the existing parallaxes should be resolved to form a coherent system for the new General Catalogue proposed by van Altena, as well as to improve luminosity calibrations and other parallax applications. Lutz has reviewed several of these problems, such as: (A) systematic differences between observatories, (B) external error estimates, (C) the absolute zero point, and (D) systematic observational effects (in right ascension, declination, apparent magnitude, etc.). Here we explore the use of cluster and spectroscopic parallaxes, and the distributions of observed parallaxes, to bring new evidence to bear on these classic problems. Several preliminary results have been obtained.


Author(s):  
P.M. Rice ◽  
MJ. Kim ◽  
R.W. Carpenter

Extrinsic gettering of Cu on near-surface dislocations in Si has been the topic of recent investigation. It was shown that the Cu precipitated hetergeneously on dislocations as Cu silicide along with voids, and also with a secondary planar precipitate of unknown composition. Here we report the results of investigations of the sense of the strain fields about the large (~100 nm) silicide precipitates, and further analysis of the small (~10-20 nm) planar precipitates.Numerous dark field images were analyzed in accordance with Ashby and Brown's criteria for determining the sense of the strain fields about precipitates. While the situation is complicated by the presence of dislocations and secondary precipitates, micrographs like those shown in Fig. 1(a) and 1(b) tend to show anomalously wide strain fields with the dark side on the side of negative g, indicating the strain fields about the silicide precipitates are vacancy in nature. This is in conflict with information reported on the η'' phase (the Cu silicide phase presumed to precipitate within the bulk) whose interstitial strain field is considered responsible for the interstitial Si atoms which cause the bounding dislocation to expand during star colony growth.


2006 ◽  
Vol 40 (12) ◽  
pp. 30
Author(s):  
BARBARA J. HOWARD
Keyword(s):  

2007 ◽  
Vol 40 (9) ◽  
pp. 36
Author(s):  
BRUCE JANCIN
Keyword(s):  

Sign in / Sign up

Export Citation Format

Share Document