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Physics News Update
Number 522, January 26, 2001 by Phil Schewe, James Riordon, and Ben Stein

Accretion Disk Around a Massive Star

We live in a relatively mature star system. Going backwards in time what one would expect to see is a gaseous accretion disk furnishing raw material for the growing protostar and for planets too at a later stage. The disk might also power jetlike outflows of material blasting away from the youthful star. Examples of such disk-star-jet systems have been seen before, but only for lightweight protostars. Now a heavyweight specimen?at 8-10 solar masses has been found.

At the recent American Astronomical Society meeting in San Diego Debra Shepard and Mark Claussen reported observations made with the Very Large Array (VLA) radio telescope of G192.16-3.82, an object about 6000 light years from Earth. To reach the extra spatial resolution needed to make out the inner disk (whose diameter, about 100 AU, is comparable to that of our solar system), the suite of 27 VLA radio dishes (each 25 m across) was joined by another dish about 32 miles away in Pie Town, New Mexico. The data from Pie Town was sent down an optical fiber as if it were a cable-TV signal, which in a way it is, and the composite antenna is (according to Claussen) the best radio telescope yet achieved for combined resolution (sharpness) and sensitivity (light-gathering ability).

The resulting view of G192's immediate vicinity suggest that not only is the protostar heavy but that the accretion disk itself is hefty (20 solar masses). Furthermore, the jets (containing an estimated 100 solar masses of material) flare outwards with a much wider opening angle (40 degrees) than for small protostars, and extend out to a distance of 15 light years in each direction.

How Random Noise Could Betray an Army's Outpost

New research adds plausibility to the notion that living things make use of random electrical noise to optimize specific behavioral responses. To test this hypothesis of "behavioral stochastic resonance," researchers have been studying the paddlefish Polyodon spathula, a primitive creature whose fossil record extends back 65 million years.

Found only in the river basins of the Midwestern United States and China's Yangtze river, the paddlefish feeds exclusively on the zooplankton Daphnia, a plankton 1-2 mm in length. Catching Daphnia mainly at the bottom of silty waters where visibility is low, the paddlefish relies upon electric-field receptors in its rostrum (a paddle-shaped nose-like appendage) to detect electric signals emitted by the plankton, whose swimming and feeding motions result in the firing of nerve cells.

In an earlier experiment (Russell et al., Nature, 18 November 1999), researchers showed that adding an intermediate amount of external noise in the vicinity of a juvenile paddlefish could improve its ability to detect and capture plankton. Now, some of the same researchers (Frank Moss, University of Missouri at St. Louis, 314-516-6150, mossf@umsl.edu and Lutz Schimansky-Geier, Humboldt University in Berlin, alsg@summa.physik.hu-berlin.de, and their colleagues) have calculated that a swarm of plankton can generate enough noise by themselves to amplify electrical signals from a single Daphnia ordinarily too weak for the paddlefish to detect, thereby betraying its presence and enabling the paddlefish to detect and capture it.

This work adds evidence to the idea that stochastic resonance has been adapted by living creatures in their evolution, and makes progress towards designing a definitive behavioral experiment to test this hypothesis. (Freund et al., Phys. Rev. E, Mar. 2001; pdf version not yet ready but we can fax the article to journalists.)