Low-mass pre--main-sequence stars in the Magellanic Clouds

[Abridged] The stellar Initial Mass Function (IMF) suggests that sub-solar stars form in very large numbers. Most attractive places for catching low-mass star formation in the act are young stellar clusters and associations, still (half-)embedded in star-forming regions. The low-mass stars in such regions are still in their pre--main-sequence (PMS) evolutionary phase. The peculiar nature of these objects and the contamination of their samples by the evolved populations of the Galactic disk impose demanding observational techniques for the detection of complete numbers of PMS stars in the Milky Way. The Magellanic Clouds, the companion galaxies to our own, demonstrate an exceptional star formation activity. The low extinction and stellar field contamination in star-forming regions of these galaxies imply a more efficient detection of low-mass PMS stars than in the Milky Way, but their distance from us make the application of special detection techniques unfeasible. Nonetheless, imaging with the Hubble Space Telescope yield the discovery of solar and sub-solar PMS stars in the Magellanic Clouds from photometry alone. Unprecedented numbers of such objects are identified as the low-mass stellar content of their star-forming regions, changing completely our picture of young stellar systems outside the Milky Way, and extending the extragalactic stellar IMF below the persisting threshold of a few solar masses. This review presents the recent developments in the investigation of PMS stars in the Magellanic Clouds, with special focus on the limitations by single-epoch photometry that can only be circumvented by the detailed study of the observable behavior of these stars in the color-magnitude diagram. The achieved characterization of the low-mass PMS stars in the Magellanic Clouds allowed thus a more comprehensive understanding of the star formation process in our neighboring galaxies.Comment: Review paper, 26 pages (in LaTeX style for Springer journals), 4 figures. Accepted for publication in Space Science Review

Development of corn seedlings after a period of exposition to various water potential

Fungicide treated and untreated corn seeds were sets to germinate under varying water availability conditions (0 to -12atm water potential). The seedlings obtained on each individual treatment were subsequently grown under ideal available water conditions. The results permitted to conclude that the occurrence of a water deficit during the on set of the germination process results in reductions on the length of the embryonic structures, particularly the epicotil. This effect attenuates with times due to the increase in growth velocity in environments where water potential is lower. Fungicid treated seeds, did not appear to be consistently vantageous in environments with water stress.Submetendo sementes de milho com e sem tratamento fungicida, a ambientes de germinação variáveis quanto à disponibilidade de água (0 a -12atm), o presente trabalho avaliou o desenvolvimento posterior das plântulas postas em ambientes sem limitações hídricas. Os resultados obtidos permitiram concluir que a ocorrência de déficit hídrico, durante o início do processo de germinação, promove reduções posteriores no comprimento das estruturas embrionárias e, de forma mais acentuada, do epicótilo; apesar disso, esse efeito se atenua com o passar do tempo pela elevação progressiva na velocidade de crescimento em ambientes que oferecem menores potenciais hídricos. Paralelamente, o tratamento fungicida das sementes pode não trazer vantagens em ambientes hidricamente deficientes; esta afirmação, contudo, considera o papel toalha como meio fornecedor de água o que, em contrapartida, exige cautela na sua extrapolação para as condições proporcionadas pelo solo