Examinando por Autor "Angelo, M."

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    The experience of nursing students in their transition to professional practice: A social phenomenological approach
    (Universidade Federal de Santa Catarina, 2011) Ramírez, A.; Angelo, M.; González, L.
    The purpose of this study was to better understand the meaning of the learning experience in transitioning from nursing student to professional, and the meaning of their expectations from their learning experience upon their future professional practice. The social phenomenological approach of Alfred Schutz was adopted in interviewing ten nursing interns. Comprehensive living experience analysis identified that the student feels that they take on suffering and uncertainty in taking on responsibility due to their lack of knowledge, lack of confidence in their abilities, and feelings of solitude. However, to the degree they perceive support they gain confidence, autonomy, and integrate themselves with the team. He/she feels, however, that nurses are important for the transition. This study made it possible to understand the reasons and motives for their actions within the transition process, as well as how a particular social group in a given time and space is integrated into the world of everyday life.
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    The VISCACHA survey-IV. the SMC West Halo in 8D
    (Oxford University Press, 2022-05-01) Dias, B.; Parisi, M.C.; Angelo, M.; Maia, F.; Oliveira, R.A.P.; Souza, S.O.; Kerber, L.O.; Santos, J.F.C.; Perez-Villegas, A.; Sanmartim, D.; Quint, B.; Fraga, L.; Barbuy, B.; Bica, E.; Santrich, O. J. Katime; Hernandez-Jimenez, J.A.; Geisler, D.; Minniti, D.; De Bórtoli, B.J.; Bassino, L.P.; Rocha, J.P.
    The structure of the Small Magellanic Cloud (SMC) is very complex, in particular in the periphery that suffers more from the interactions with the Large Magellanic Cloud (LMC). A wealth of observational evidence has been accumulated revealing tidal tails and bridges made up of gas, stars, and star clusters. Nevertheless, a full picture of the SMC outskirts is only recently starting to emerge with a 6D phase-space map plus age and metallicity using star clusters as tracers. In this work, we continue our analysis of another outer region of the SMC, the so-called West Halo, and combined it with the previously analysed Northern Bridge. We use both structures to define the Bridge and Counter-bridge trailing and leading tidal tails. These two structures are moving away from each other, roughly in the SMC-LMC direction. The West Halo form a ring around the SMC inner regions that goes up to the background of the Northern Bridge shaping an extended layer of the Counter-bridge. Four old Bridge clusters were identified at distances larger than 8 kpc from the SMC centre moving towards the LMC, which is consistent with the SMC-LMC closest distance of 7.5 kpc when the Magellanic Bridge was formed about 150Myr ago; this shows that the Magellanic Bridge was not formed only by pulled gas, but it also removed older stars from the SMC during its formation. We also found age and metallicity radial gradients using projected distances on sky, which are vanished when we use the real 3D distances. © 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.