The First Empirical Mass Loss Law for Population II Giants

Using the Spitzer IRAC camera we have obtained mid-IR photometry of the red giant branch stars in the Galactic globular cluster 47 Tuc. About 100 stars show an excess of mid-infrared light above that expected from their photospheric emission. This is plausibly due to dust formation in mass flowing from these stars. This mass loss extends down to the level of the horizontal branch and increases with luminosity. The mass loss is episodic, occurring in only a fraction of stars at a given luminosity. Using a simple model and our observations we derive mass loss rates for these stars. Finally, we obtain the first empirical mass loss formula calibrated with observations of Population II stars. The dependence on luminosity of our mass loss rate is considerably shallower than the widely used Reimers Law. The results presented here are the first from our Spitzer survey of a carefully chosen sample of 17 Galactic Globular Clusters, spanning the entire metallicity range from about one hundredth up to almost solar. Subject headings: stars: Population II, mass loss – circumstellar matter – infrared: stars 1 This work is based on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. Support for this work was provided by NASA through an award issued by JPL/Caltech. INAF–Osservatorio Astronomico di Bologna, Via Ranzani 1, I–40127 Bologna, Italy, livia.origlia oabo.inaf.it, flavio.fusipecci oabo.inaf.it Astronomy Department, University of Virginia, Charlottesville, VA 22903, rtr virginia.edu Università degli Studi di Bologna, Dip. di Astronomia, Via Ranzani 1, I–40127 Bologna, Italy, sara.fabbri studio.unibo.it,francesco.ferraro3 unibo.it 5 Department of Physics and Astronomy, University of California at Los Angeles, Los Angeles, CA 900951547, rmr astro.ucla.edu