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Author |
Hauswald, H.; Hack, A.; Kellermanns, F.W.; Patzelt, H. |
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Title |
Attracting New Talent to Family Firms: Who Is Attracted and Under What Conditions? |
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Journal Article |
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Year |
2015 |
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Entrepreneurship Theory and Practice |
Abbreviated Journal |
Entrepreneurship Theory and Practice |
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n/a-n/a |
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In making a decision to enter into a long-term employment relationship with a firm, job seekers often compare their needs and values with the perceived organizational characteristics of the firm. In the case of family firms, the communication of family influence can be a unique factor in shaping beliefs about firm attributes. Family influence is often associated with trustworthiness, security, and stability. However, family influence is also associated with inflexibility and resistance to change. Using the idea of person–organization fit, we hypothesize that although family influence attracts job seekers in general, applicants who value conservation or self-transcendence are particularly attracted, while applicants who emphasize openness to change or self-enhancement are less attracted. Furthermore, we propose that the attractive effects of family influence are more pronounced in more hostile economic environments. We find evidence for our hypotheses using a conjoint experiment and 5,600 assessments of family influence nested within 175 job seekers. |
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1540-6520 |
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ATM @ robstephens13 @ |
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41747 |
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Author |
Jaskiewicz, P.; Heinrichs, K.; Rau, S.B.; Reay, T. |
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Title |
To Be or Not to Be: How Family Firms Manage Family and Commercial Logics in Succession |
Type |
Journal Article |
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Year |
2015 |
Publication |
Entrepreneurship Theory and Practice |
Abbreviated Journal |
Entrepreneurship Theory and Practice |
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n/a-n/a |
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We draw on the institutional logics perspective to understand different approaches that family firms can use to manage the process of succession. Based on the analysis of 21 case studies of family firms in Germany, we identify four different ways of managing potentially conflicting family and commercial logics that are associated with four different succession processes. Our findings contribute to the family firm literature by improving our knowledge of the heterogeneity of family firms and by explaining different ways that the family logic can influence firm behavior. Moreover, we contribute to institutional theory by showing the importance of filtering mechanisms for organizations that must respond to coexisting logics. |
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1540-6520 |
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ATM @ robstephens13 @ |
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41768 |
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Sargent, B.A.; Srinivasan, S.; Speck, A.; Volk, K.; Kemper, C.; Reach, W.T.; Lagadec, E.; Bernard, J.-P.; McDonald, I.; Meixner, M. |
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Spitzer-IRS Spectroscopic Studies of Oxygen-Rich Asymptotic Giant Branch Star and Red Supergiant Star Dust Properties |
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Conference Article |
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2015 |
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216.03-216.03 |
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American Astronomical Society Meeting Abstracts |
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225 |
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proceedings |
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ASIAA @ ciska @ |
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41812 |
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Sloan, G.C.; Groenewegen, M.; Srinivasan, S.; Lagadec, E.; Kraemer, K.E.; McDonald, I.; Boyer, M.L.; Zijlstra, A.; Kemper, C. |
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Title |
Dust and metallicity in carbon stars |
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Conference Article |
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Year |
2015 |
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216.04-216.04 |
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American Astronomical Society Meeting Abstracts |
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225 |
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proceedings |
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ASIAA @ ciska @ |
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41813 |
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Ruffle, P.M.E.; Kemper, F.; Jones, O.C.; Sloan, G.C.; Kraemer, K.E.; Woods, P.M.; Boyer, M.L.; Srinivasan, S.; Antoniou, V.; Lagadec, E.; Matsuura, M.; McDonald, I.; Oliveira, J.M.; Sargent, B.A.; Sewiło, M.; Szczerba, R.; van Loon, J.T.; Volk, K.; Zijlstra, A.A. |
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Title |
Spitzer infrared Spectrograph point source classification in the Small Magellanic Cloud |
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Journal Article |
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2015 |
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Mon.~Not.~R.~Astron.~Soc. |
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submitted; Owner: ciska; Added to JabRef: 2015.03.04 |
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Call Number |
ASIAA @ ciska @ |
Serial |
41816 |
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Zhao-Geisler, R.; Köhler, R.; Kemper, F.; Kerschbaum, F.; Mayer, A.; Quirrenbach, A.; Lopez, B. |
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Title |
Spectro-imaging of the asymmetric inner molecular and dust shell region of the Mira variable W Hya with MIDI/VLTI |
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Journal Article |
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2015 |
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Pub.~Astron.~Soc.~Pacific |
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We have observed W Hya, one of the closest and best studied oxygen-rich evolved star, in the dust |
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submitted; Owner: ciska; Added to JabRef: 2015.04.15 |
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ASIAA @ ciska @ |
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41817 |
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Ruffle, P.M.E.; Kemper, F.; Jones, O.C.; Sloan, G.C.; Kraemer, K.E.; Woods, P.M.; Boyer, M.L.; Srinivasan, S.; Antoniou, V.; Lagadec, E.; Matsuura, M.; McDonald, I.; Oliveira, J.M.; Sargent, B.A.; Sewiło, M.; Szczerba, R.; van Loon, J.T.; Volk, K.; Zijlstra, A.A. |
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Title |
Spitzer infrared Spectrograph point source classification in the Small Magellanic Cloud |
Type |
Journal Article |
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Year |
2015 |
Publication |
Mon.~Not.~R.~Astron.~Soc. |
Abbreviated Journal |
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submitted; Owner: ciska; Added to JabRef: 2015.03.04 |
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ASIAA @ ciska @ |
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42053 |
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Sargent, B.A.; Srinivasan, S.; Speck, A.; Volk, K.; Kemper, C.; Reach, W.T.; Lagadec, E.; Bernard, J.-P.; McDonald, I.; Meixner, M. |
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Title |
Spitzer-IRS Spectroscopic Studies of Oxygen-Rich Asymptotic Giant Branch Star and Red Supergiant Star Dust Properties |
Type |
Conference Article |
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Year |
2015 |
Publication |
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216.03-216.03 |
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Abstract |
We analyze the dust emission features seen in Spitzer Space Telescope Infrared Spectrograph (IRS) spectra of Oxygen-rich (O-rich) asymptotic giant branch (AGB) and red supergiant (RSG) stars. The spectra come from the Spitzer Legacy program SAGE-Spectroscopy (PI: F. Kemper) and other archival Spitzer-IRS programs. The broad 10 and 20 micron emission features attributed to amorphous dust of silicate composition seen in the spectra show evidence for systematic differences in the centroid of both emission features between O-rich AGB and RSG populations. Radiative transfer modeling using the GRAMS grid of models of AGB and RSG stars suggests that the centroid differences are due to differences in dust properties. We present an update of our investigation of differences in dust composition, size, shape, etc that might be responsible for these spectral differences. We explore how these differences may arise from the different circumstellar environments around RSG and O-rich AGB stars. BAS acknowledges funding from NASA ADAP grant NNX13AD54G. |
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American Astronomical Society Meeting Abstracts |
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225 |
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proceedings; Owner: ciska; Added to JabRef: 2015.04.16 |
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Call Number |
ASIAA @ ciska @ |
Serial |
42059 |
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Author |
Sloan, G.C.; Groenewegen, M.; Srinivasan, S.; Lagadec, E.; Kraemer, K.E.; McDonald, I.; Boyer, M.L.; Zijlstra, A.; Kemper, C. |
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Title |
Dust and metallicity in carbon stars |
Type |
Conference Article |
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Year |
2015 |
Publication |
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Abbreviated Journal |
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Volume |
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Issue |
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216.04-216.04 |
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Abstract |
The Infrared Spectrograph on the Spitzer Space Telescope observed over 200 carbon stars in nearby metal-poor dwarf galaxies. These spectra probe how the quantity and composition of dust produced by carbon stars depend on initial metallicity, initial mass, and pulsational properties. For stars to produce significant quantities of dust, they must be pulsating in the fundamental mode with strong amplitudes. The spectra confirm that carbon stars with longer pulsation periods produce more dust and that the amount of dust shows no strong dependence on metallicity. This sample includes more carbon stars with low mass and reveals that for a given pulsation period, higher-mass stars produce less dust. Evidence is building for the layering of dust grains, with SiC cores in grains produced by metal-rich carbon stars, and mantles of MgS around grains in all embedded stars. |
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Abbreviated Series Title |
American Astronomical Society Meeting Abstracts |
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Series Volume |
225 |
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proceedings; Owner: ciska; Added to JabRef: 2015.04.16 |
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Call Number |
ASIAA @ ciska @ |
Serial |
42063 |
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Author |
Zhao-Geisler, R.; Köhler, R.; Kemper, F.; Kerschbaum, F.; Mayer, A.; Quirrenbach, A.; Lopez, B. |
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Title |
Spectro-imaging of the asymmetric inner molecular and dust shell region of the Mira variable W Hya with MIDI/VLTI |
Type |
Journal Article |
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Year |
2015 |
Publication |
Pub.~Astron.~Soc.~Pacific |
Abbreviated Journal |
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my_papers |
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Abstract |
We have observed W Hya, one of the closest and best studied oxygen-rich evolved star, in the dust |
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submitted; Owner: ciska; Added to JabRef: 2015.04.15 |
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Call Number |
ASIAA @ ciska @ |
Serial |
42091 |
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