The Chandra Carina Complex Project
Friday, May 13, 2011
Science Update - A look at CfA discoveries from recent journals

The Great Nebula in the constellation of Carina is a massive star-forming complex located about 7.5 thousand light-years away. The main star in the complex, Eta Carinae, shines brightly in the southern sky. Its ensemble of stellar clusters are young and hot, with ages that range from less than about one million years to about six million years. Altogether, the region contains one of the richest concentrations of massive young stars in the galaxy. In addition, the region is rich in non-stellar material including filaments, pillars, cavities, arcs, and other features indicative of a turbulent and complex history.

The Nebula is not only rich in hot sources. It is also full of mysteries because the numerous complex structures have proven difficult to explain. Some scientists think there has been an early epoch of active star formation in the region, and whether or not a supernova may have gone off in the neighborhood (and so generated some of the observed structures) is actively debated. The role of intense shocks and colliding winds in generating the hot diffuse gas that is seen is also controversial.

A large team of CfA astronomers and their colleagues has used the Chandra X-ray Observatory to study the Great Nebula in Carinae, integrating new data with older observations from the Chandra archives. They have begun publishing a landmark set of sixteen papers on the region and its rich astrophysical contents, including separate studies of its massive stars, intermediate mass stars, and low mass stars, magnetic field effects, and the infrared characteristics of its dust enshrouded sources.

One of the new papers examines the X-ray emission from the hottest, most massive stars in the cluster, of which 68 (of the 70 known) were detected in this study. It has long been thought that shocks from powerful winds produce X-ray emission; this is in contrast to smaller stars whose photospheres can produce X-ray emission. This new study finds that there appear to be at least three different kinds of shocks at work: those embedded in the stellar wind, others due to collisions between the winds from two massive stars that orbit each other in a binary pair, and shocks produced when magnetically channeled winds from the opposite hemispheres of a star meet and collide. Other results of this survey include a catalog of over 14,000 X-ray point sources, mostly stars. The set of new papers represents a basic reference for understanding this famous beacon in the southern sky and the mechanisms at work generating stellar X-rays.