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Corporate Use of Social Media during Food Product Harm Crises: Exploring the “Social Nature” of Product Recalls W. Timothy Coombs* and Sherry J. Holladay Department of Communication Texas A&M University Corporate Use of Social Media during Food Product Harm Crises: Exploring the “Social Nature” of Product Recalls Research in crisis communication frequently focuses on atypical, dramatic crises such

https://www.isk.lu.se/sites/isk.lu.se/files/tomothy_coombs_sherry_j_holladay.pdf - 2026-05-31

MOBILITY AND TRANSPORT: INDIVIDUAL AND SOCIETAL CONCEPTUALIZATIONS ON PRIVATE CAR PURCHASE AND USE (A Case Study of Car Consumption in the City of Lagos, Nigeria) A Thesis Presented in Partial Fulfilment of the Requirements Of the Lund University International Master Programme in Environmental Science LUND UNIVERSITY, SWEDEN 21 November 2005 CHIJIOKE DIKE UBA Lumes 2004/2005 e-mail : dikeuba@yahoo

https://www.lumes.lu.se/sites/lumes.lu.se/files/chijioke_uba.pdf - 2026-05-31

The use of Alcohol-based antiseptics is efficient and approved, however it has some limitations. This paper examined the possibility of using hypochlorite water as a chlorine-based antiseptic for handwashing in public buildings and healthcare facilities. The electrolysis method was used, which produces Hypochlorous acid (HOCl) from mixing drinking water with small amounts of sodium hydroxide. Hypo

We analyse N-body simulations of star-forming regions to investigate the effects of externalfar- and extreme-ultraviolet photoevaporation from massive stars on protoplanetary discs. Byvarying the initial conditions of simulated star-forming regions, such as the spatial distribution,net bulk motion (virial ratio), and density, we investigate which parameters most affect the rateat which discs are d

Most stars form in a clustered environment. Both single and binary stars will sometimes encounter planetary systems in such crowded environments. Encounter rates for binaries may be larger than for single stars, even for binary fractions as low as 10-20 per cent. In this work, we investigate scatterings between a Sun-Jupiter pair and both binary and single stars as in young clusters.We first perfo

This article is over 5 years old, and the information may therefore be outdated. A person who carries the mutant gene will at some point in his or her life develop the deadly Huntington's disease. This brain disease can be inherited from generation to generation and begins insidiously, making it increasingly difficult to regulate emotions, thoughts, then movements. There is no treatment that slows

https://www.medicine.lu.se/article/huntingtons-disease-fascinating-and-touching-mystery - 2026-05-29

pedi_774.dvi Pediatric Diabetes 2011 doi: 10.1111/j.1399-5448.2011.00774.x All rights reserved © 2011 John Wiley & Sons A/S Pediatric Diabetes Original Article The Environmental Determinants of Diabetes in the Young (TEDDY): genetic criteria and international diabetes risk screening of 421 000 infants Hagopian WA, Erlich H, Lernmark Å, Rewers M, Ziegler AG, Simell O, Akolkar B, Vogt Jr R, Blair A

https://www.teddy.lu.se/sites/teddy.lu.se/files/06032016_679_13_hagopian_ped_diab_2011.pdf - 2026-05-31

Supermassive black holes (SMBHs) are found in most galactic nuclei. A significant fraction of these nuclei also contains a nuclear stellar cluster (NSC) surrounding the SMBH. In this paper, we consider the idea that the NSC forms first, from the merger of several stellar clusters that may contain intermediate-mass black holes (IMBHs). These IMBHs can subsequently grow in the NSC and form an SMBH.

Professorsinstallation LUNDS UNIVERSITET | AULAN | 6 OKTOBER 2017 KL 16.00 Denna broschyr finns på installandis institutioner och kan också beställas från sektionen Kommunikation, tel 046-222 70 10, e-post info@kommunikation.lu.se. Broschyren finns även på www.lu.se/om-universitetet/akademiska-hogtider/professorsinstallationer Produktion Sektionen Kommunikation och Media-Tryck, Lunds universitet F

https://www.lu.se/sites/www.lu.se/files/professorsinstallation-lunds-universitet-6okt2017.pdf - 2026-05-31

Professorsinstallation LUNDS UNIVERSITET | AULAN | 6 OKTOBER 2017 KL 16.00 Denna broschyr finns på installandis institutioner och kan också beställas från sektionen Kommunikation, tel 046-222 70 10, e-post info@kommunikation.lu.se. Broschyren finns även på www.lu.se/om-universitetet/akademiska-hogtider/professorsinstallationer Produktion Sektionen Kommunikation och Media-Tryck, Lunds universitet F

https://www.lu.se/sites/www.lu.se/files/professorsinstallation6okt2017-lunds-universitet.pdf - 2026-05-31

lum_2006_08 LUM Lunds universitets magasin | Nr 8 | 2006 sLäkten är bäst! Inredningspengar tog slut på SOL Politikerfritt i styrelsen? LUM nr 8 | 2006 MersMak LUM nr 8 | 2006 Det gick åt cirka 0 kilo choklad för att hålla igång den mörkt drop- pande chokladfontänen som blev många barns höjdpunkt under Ve- tenskapskarnevalen. Kakao var te- mat i den deckargåta som främst mellanstadiebarn från hel

https://www.lu.se/sites/www.lu.se/files/lunds-universitets-magasin-8-2006.pdf - 2026-05-31

We investigate the possibility of finding Earth-like planets in the habitable zone of 34 nearby FGK-dwarfs, each known to host one giant planet exterior to their habitable zone detected by RV. First we simulate the dynamics of the planetary systems in their present day configurations and determine the fraction of stable planetary orbits within their habitable zones. Then, we postulate that the ecc

Primordial black holes formed through the collapse of cosmological density fluctuations have been hypothesized as contributors to the dark matter content of the Universe. At the same time, their mergers could contribute to the recently observed population of gravitational-wave sources. We investigate the scenario in which primordial black holes form binaries at late times in the Universe. Specific

LUM Lunds universitets magasin | Nr 2 | 2009 TeaMbUiLding! Utbildnings­ frågor högt på agendan Nytt hopp om bot mot förkylning 2 LUM nr 2 | 2009 sTjärngossen LUM nr 2 | 2009 3 Inför en fullsatt universitetsaula över- lämnade rektor emeritus Göran Bexell universitetsregalierna till den tillträ- dande rektorn. – Du bär kedjan inte bara i fram- gång, utan även i motgång, sa den av- gående rektorn när

https://www.lu.se/sites/www.lu.se/files/lunds-universitets-magasin-2-2009.pdf - 2026-05-31

1 Lunds universitet Institutionen för Öst- och Centraleuropastudier Ht 2005 Handledare: Sanimir Resic Det jugoslaviska sammanbrottet En analys av skuldfrågan avseende den jugoslaviska statens sönderfall i början av 1990-talet Peter Ekström 1 Sammanfattning Förevarande uppsats syftar till att belysa frågan huruvida det är möjligt att finna en part såsom ansvarig för den jugoslaviska statens sönderf

https://www.sol.lu.se/fileadmin/user_upload/amnen/ocek/PeterEkstrom.pdf - 2026-05-30

Microsoft Word - Idris_Thesis_livelihoods_.doc A socio-economic sustainability assessment of livelihoods from scrap metal collection in Freetown, Sierra Leone. Idris Nabih Fofana naidris27@yahoo.com Thesis Supervisor: Barry Ness (PhD) barry.ness@lucsus.lu.se Lund University Center for Sustainability Studies (LUCSUS) Geocentrum 1, Solvagatan 10, P.O.Box 170, SE-221 00 Lund, Sweden. Phone: +46 (0) 4

https://www.lumes.lu.se/sites/lumes.lu.se/files/fofana_idris_1.pdf - 2026-05-31

The 4MOST consortium is currently halfway through a Conceptual Design study for ESO with the aim to develop a wide-field (>3 square degree, goal >5 square degree), high-multiplex (>1500 fibres, goal 3000 fibres) spectroscopic survey facility for an ESO 4m-class telescope (VISTA). 4MOST will run permanently on the telescope to perform a 5 year public survey yielding more than 20 million spectra at

The stellar-to-halo mass relation (SHMR) is not only one of the main sources of information we have on the connection between galaxies and their dark matter haloes, but also an important indicator of the performance of galaxy formation models. Here, we use one of the largest sample of galaxies with both high-quality rotation curves and near-infrared surface photometry, and perform a detailed compa

We introduce a new method to mitigate numerical diffusion in adaptive mesh refinement (AMR) simulations of cosmological galaxy formation, and study its impact on a simulated dwarf galaxy as part of the 'EDGE' project. The target galaxy has a maximum circular velocity of 21 km s-1 but evolves in a region that is moving at up to 90 km s-1 relative to the hydrodynamic grid. In the absence of any miti