Resistance to Change and Conflict of Interest: A Case Study

Change for organizations is a necessity. Today’s businesses are aware of the need to keep up with the environmental changes and change demands. If the change process is not handled properly in the business, it will bring major problems with it. Every change will absolutely and definitely face resistance. Similarly, conflicts are considered to be inherent in organizations. The important thing is to prevent conflicts from taking over organizational interests. If conflicts arise in situations where personal interests constitute a source, it is an issue that needs to be discussed seriously. This study is intended to reveal elements that create a potentially resilient potential, in particular protecting personal interests. A case study method was utilized in the study. This method is preferred because it is appropriate to examine in detail the history, current situation and environmental functioning of a particular person or group and to obtain appropriate information in order to provide statistical methods. In particular, the case study, which reveals a reflection of the conflict of interest that is valued as a consequence of the functions of exchange resistance and as a consequence thereof, reflects the relationship between resistance and conflict of interest

Star formation in the outer regions of the early type galaxy NGC 4203

NGC 4203 is a nearby early-type galaxy surrounded by a very large, low-column-density HI disc. In this paper we study the star formation efficiency in the gas disc of NGC 4203 by using the UV, deep optical imaging and infrared data. We confirm that the HI disc consists of two distinct components: an inner star forming ring with radius from $\sim$ 1 to $\sim$ 3 R$_{eff}$, and an outer disc. The outer HI disc is 9 times more massive than the inner HI ring. At the location of the inner HI ring we detect spiral-like structure both in the deep $g'-r'$ image and in the 8 $\mu$m $Spitzer$-IRAC image, extending in radius up to $\sim$ 3 R$_{eff}$. These two gas components have a different star formation efficiency likely due to the different metallicity and dust content. The inner component has a star formation efficiency very similar to the inner regions of late-type galaxies. Although the outer component has a very low star formation efficiency, it is similar to that of the outer regions of spiral galaxies and dwarfs. We suggest that these differences can be explained with different gas origins for the two components such as stellar mass loss for the inner HI ring and accretion from the inter galactic medium (IGM) for the outer HI disc. The low level star formation efficiency in the outer HI disc is not enough to change the morphology of NGC 4203, making the depletion time of the HI gas much too long.Comment: Accepted for publication in MNRAS. 12 pages, 7 figure

Glueballs, gluerings and gluestars in the d=2+1 SU(N) gauge theory

The 3d gluodynamics which governs the large T quark gluon plasma is studied in the framework of the field correlator method. Field correlators and spacial string tension are derived through the gluelump Green's functions. The glueball spectrum is calculated both in C=-1 as well as in C=+1 sectors, and multigluon bound states in the form of "gluon rings" and "gluon stars" are computed explicitly. Good overall agreement with available lattice data is observed.Comment: 19 page

The ATLAS3D project - XXIX : The new look of early-type galaxies and surrounding fields disclosed by extremely deep optical images

Date of Acceptance: 25/09/2014Galactic archaeology based on star counts is instrumental to reconstruct the past mass assembly of Local Group galaxies. The development of new observing techniques and data reduction, coupled with the use of sensitive large field of view cameras, now allows us to pursue this technique in more distant galaxies exploiting their diffuse low surface brightness (LSB) light. As part of the ATLAS3D project, we have obtained with the MegaCam camera at the Canada-France-Hawaii Telescope extremely deep, multiband images of nearby early-type galaxies (ETGs). We present here a catalogue of 92 galaxies from the ATLAS3D sample, which are located in low- to medium-density environments. The observing strategy and data reduction pipeline, which achieve a gain of several magnitudes in the limiting surface brightness with respect to classical imaging surveys, are presented. The size and depth of the survey are compared to other recent deep imaging projects. The paper highlights the capability of LSB-optimized surveys at detecting new prominent structures that change the apparent morphology of galaxies. The intrinsic limitations of deep imaging observations are also discussed, among those, the contamination of the stellar haloes of galaxies by extended ghost reflections, and the cirrus emission from Galactic dust. The detection and systematic census of fine structures that trace the present and past mass assembly of ETGs are one of the prime goals of the project. We provide specific examples of each type of observed structures - tidal tails, stellar streams and shells - and explain how they were identified and classified. We give an overview of the initial results. The detailed statistical analysis will be presented in future papers.Peer reviewedFinal Accepted Versio

İngilizce Wikipedia makalelerinden bilgi kutuları için anlamsal çıkarım modeli geliştirilmesi

With the beginning of internet era in the mid '90s, the source of knowledge started to change rapidly from written sources such as the well-known Enyclopedia Britannica to online sources. One of the first online sources of the free encyclopedia was called Interpedia would let anyone contribute by writing articles and submitting to the database to published which is very similar with "Wikipedia", today's most used online & free encyclopedia

İzole kurbağa üst özofagus dairevi kas şeritlerinde süper oksit anyon radikallerinin etkisi

TEZ2084Tez (Yüksek Lisans) -- Çukurova Üniversitesi, Adana, 1996.Kaynakça (s. 46-48) var.vii, 48 s. ; 30 cm.

Homosistein'in sıçan torasik aortasında nitrerjik gevşemeler üzerindeki etkisi

TEZ3742Tez (Doktora) -- Çukurova Üniversitesi, Adana, 2001.Kaynakça (s. 41-47) var.x, 48 s. ; 30 cm.…Bu çalışma Ç.Ü. Bilimsel Araştırma Projeleri Birimi Tarafından Desteklenmiştir. Proje No: SBE. 98. D. 6