The recent growth and development of the multinational corporation presents the international community with a unique challenge. For the first time man has an instrument which enables him to use the world's resources with maximum efficiency. He is no longer restricted by national boundaries, but is able to allocate resources on a world wide basis. In addition, the multinational enterprise provides a means for linking the developing countries to an international productive scheme. These countries are now able to undertake production of goods in which they have a comparative advantage and more rapidly increase their rate of economic development.Since the multinational enterprise trains the manpower of nations, develops their resources, and permits a cross fertilization of ideas and cultures, it may also be an important element in reconciling the diverse peoples of the world. Indeed, some observers believe that the multinational corporation will be more than merely an instrument for production; it will be "a stabilizer in a world full of tensions,"' and provide "a means of unifying and reconciling the aspirations of mankind . " The internationalization of the activities of the modern corporation is, however, challenging the legal and political monopoly of the nation state.
Background: Acharacteristic feature of cancer is, among other things, that even after successful oncological treatment, the patient cannot close this chapter of life and the experience of being acancer patient. In oncology there is no unambiguous definition of apatient as ahealthy person. Methods: The study covered agroup of 20 people. In the con- ducted tests the diagnostic survey method was introduced. The technique of individual in-depth interviews was used. The re- spondent could fully express his or her own feelings, emotions, thoughts and experiences. Results. The respondents stated that positive emotions ap- peared with the completion of treatment, but indicated that the feelings were not related to the sense of healing but only to the completion of tiring therapeutic procedures. Some respondents complained about the feeling of chronic fatigue. Fatigue was not only related to the physical sphere, although everyone con- firmed that the side effects of the therapy persisted for some time. The respondents paid more attention to mental fatigue, which had various forms, e.g.: anxiety about possible relapse; functional losses; feeling of loss caused by radical treatment. Out of 20 respondents, 4 persons indicated aloss of health, es- pecially the sense of joy and happiness, self-esteem, self-con- fidence, social contacts, family and time. Conclusions: The research group consisted of 20 respondents, which limits the possibility of formulating generalized con- clusions, but indicates various directions of possible improve- ment and, most importantly, shows how the thinking about can- cer can be changed.
We report the discovery of a Neptune-like planet (LP 714-47 b, P = 4.05204 d, mb = 30.8 ± 1.5Mpdbl, Rb = 4.7 ± 0.3 Rpdbl) located in the "hot Neptune desert". Confirmation of the TESS Object of Interest (TOI 442.01) was achieved with radial-velocity follow-up using CARMENES, ESPRESSO, HIRES, iSHELL, and PFS, as well as from photometric data using TESS, Spitzer, and ground-based photometry from MuSCAT2, TRAPPIST-South, MONET-South, the George Mason University telescope, the Las Cumbres Observatory Global Telescope network, the El Sauce telescope, the TÜBITAK National Observatory, the University of Louisville Manner Telescope, and WASP-South. We also present high-spatial resolution adaptive optics imaging with the Gemini Near-Infrared Imager. The low uncertainties in the mass and radius determination place LP 714-47 b among physically well-characterised planets, allowing for a meaningful comparison with planet structure models. The host star LP 714-47 is a slowly rotating early M dwarf (Teff = 3950 ± 51 K) with a mass of 0.59 ± 0.02Mpdbl and a radius of 0.58 ± 0.02Rpdbl. From long-term photometric monitoring and spectroscopic activity indicators, we determine a stellar rotation period of about 33 d. The stellar activity is also manifested as correlated noise in the radial-velocity data. In the power spectrum of the radial-velocity data, we detect a second signal with a period of 16 days in addition to the four-day signal of the planet. This could be shown to be a harmonic of the stellar rotation period or the signal of a second planet. It may be possible to tell the difference once more TESS data and radial-velocity data are obtained. ; With funding from the Spanish government through the "María de Maeztu Unit of Excellence" accreditation (MDM-2017-0737)
