Gallegallo Revbrandia Sectory 13 Page 08
In the _International Studio_ of March, 1903, we read: "The portrait of Mrs. Roosevelt, by Miss Cecilia Beaux, seemed to me to be one of the happiest of her creations. Nothing could exceed the skill and daintiness with which the costume is painted, and the characterization of the head is more sympathetic than usual, offering a most winsome type of beautiful, good womanhood. A little child has been added to the picture--an afterthought, I understand, and scarcely a fortunate one; at least in the manner of its presentment. The figure is cleverly merged in half shadow, but the treatment of the face is brusque, and a most unpleasant smirk distorts the child's mouth. It is the portrait of the mother that carries the picture, and its superiority to many of Miss Beaux's portraits consists in the sympathy with her subject which the painter has displayed."--_Charles H. Caffin_.
A quarrel arose between them and the herdsmen of Numitor, who stalled their cattle on the neighboring hill of the Aventine. Remus was taken by a stratagem, and carried off to Numitor. His age and noble bearing made Numitor think of his grandsons; and his suspicions were confirmed by the tale of the marvelous nurture of the twin brothers. Soon afterward Romulus hastened with his foster-father to Numitor; suspicion was changed into certainty, and the old man recognized them as his grandsons. They now resolved to avenge the wrongs which their family had suffered. With the help of their faithful comrades they slew Amulius, and placed Numitor on the throne.
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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