Physics
Scientific paper
Dec 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999sf99.proc..322s&link_type=abstract
Star Formation 1999, Proceedings of Star Formation 1999, held in Nagoya, Japan, June 21 - 25, 1999, Editor: T. Nakamoto, Nobeyam
Physics
Scientific paper
By filtering out the straight filaments of the Galactic Cente Arc in VLA radio images of Yusef-Zadeh and Morris, we show that numerous concentric radio shells and arcs of radii 5 to 10 pc are coherently surrounding the Pistol and Sickle region. Each shell has a thermal energy of the order of 1049 ergs. Several CO-line shells are found toward the radio shells with kinetic energy of the order of 1049-50 ergs. We propose a new idea that the concentric shell structure has the common origin: they are expanding fronts from intermittent outflows and/or ionization due to successive star-forming activities near to the Pistol and Quintuplet stars.
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