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Possible triggered star formation associated with SNR G59.5+0.1
Published online by Cambridge University Press: 21 March 2013
Abstract
We perform the submillimeter/millimeter observations in CO lines toward the southeast of SNR G59.5+0.1 with the KOSMA 3m-Telescope, which fully covers the open cluster NGC 6823. Three molecular clumps are identified in the CO molecular arc, each clump show outflow in motion. The age of the SNR is 8.6×104 yr. The number of selected YSOs are significantly enhanced in the interacting regions, indicating the presence of some recently formed stars.
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- Copyright © International Astronomical Union 2013
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