A Comment on the March Moscow Meeting by Hongqi Renmin Ribao

By Hongqi Renmin Ribao

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Stirring the Pot T H E O U T L I N E S O F fruitful theories for the shaping of planetary nebulae continue to emerge. The trick is to develop models that embrace the entire vexing array of observations. Researchers now agree that one of the principal players is the gravitational influence of companion stars. At least 50 percent of all the “stars” you see at night are really pairs of stars orbiting each other. In most of these systems, the stars are so far apart that they develop independently. But in a small fraction, the gravity of one star can deflect or even control the material flowing out of another.

We did not attempt to explain why the slow wind would be ejected as a torus, hoping that particular detail would be filled in later. Our confidence in the model was quickly deflated. In 1994 Hubble took its first clear image of a planetary nebula, the Cat’s Eye (designated NGC 6543), first seen by Herschel. That fateful picture blew us off our chairs. One of its two crossed ellipses, a thin rim surrounding an ellipsoidal cavity, matched the model. But what were all those other structures? No one had predicted that clumpy redcolored regions would lace the nebula; 56 jetlike streaks immediately outside it were stranger still.

My own work began with observing members of my family, many of whom lived well into their 80s and 90s. Although they enjoyed RESEARCH TOWARD in all mammals and probably results from a cumulative failure to repair damage caused by normal use. Intriguingly, aging-related changes in skeletal muscle resemble the functional and physical changes seen in a suite of diseases collectively known as muscular dystrophy, albeit at a much slower rate. In the most common and most severe version of MD— Duchenne muscular dystrophy— an inherited gene mutation results in the absence of a protein called dystrophin that protects muscle fibers from injury by the force they exert during regular movement.

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