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Zaproburno Yollanica Directory 15
Page 10
The leaders of the popular party perceived the mistake they had made in alienating the Italians from their cause, and they now secured their adhesion by offering them the Roman citizenship if they would support the Agrarian Law. As Roman citizens they would, of course, be entitled to the benefits of the law, while they would, at the same time, obtain what they had so long desired--an equal share in political power. But the existing citizens, who saw that their own importance would be diminished by an increase in their numbers, viewed such a proposal with the utmost repugnance. So strong was their feeling that, when great numbers of the Italians had flocked to Rome in B.C. 126, the Tribune M. Junius Pennus carried a law that all aliens should quit the city.
BRACKEN, JULIA M. First prize for sculpture, Chicago, 1898; appointed on staff of sculptors for the St. Louis Exposition. Member of Arts Club, Western Society of Artists, Municipal Art League, and Krayle Workshop, Chicago. Born at Apple River, Ill., 1871. Pupil of Chicago Art Institute. Acted as assistant to Lorado Taft, 1887-92. Was much occupied with the decorations for the Columbian Exposition, and executed on an independent commission the statue of "Illinois Welcoming the Nations." There are to be five portrait statues placed in front of the Educational Building at St. Louis, each to be executed by a well-known artist. One of these is to be the work of Miss Bracken, who is the only woman among them. Miss Bracken has modelled an heroic portrait statue of President Monroe; beside the figure is a globe, on which he points out the junction of the Mississippi and Missouri rivers.
It acquires a yellowish tinge. As it continues to contract it grows hotter and hotter until its temperature reaches a maximum as a white star. At this point the contraction process does not stop, but the heating process does. Further contraction is now accompanied by cooling, and the star goes through its colour changes again, but this time in the inverse order. It contracts and cools to yellow and finally to red. But when it again becomes a red star it is enormously denser and smaller than when it began as a red star. Consequently the red stars are divided into two classes called, appropriately, Giants and Dwarfs. This theory, which we owe to an American astronomer, H. N. Russell, has been successful in explaining a variety of phenomena, and there is consequently good reason to suppose it to be true. But the question as to how the red giant stars were formed has received less satisfactory and precise answers.
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