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Possible triggered star formation associated with SNR G59.5+0.1

Published online by Cambridge University Press:  21 March 2013

Jin-Long Xu  and
Jun-Jie Wang
Jin-Long Xu
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, 100012 Beijing, China; email: xujl@bao.ac.cn
Jun-Jie Wang
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, 100012 Beijing, China; email: xujl@bao.ac.cn
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Abstract

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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.

Keywords

ISM: clouds — ISM: individual (G59.5+0.1) — ISM: molecules — stars: formation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S292: Molecular Gas, Dust, and Star Formation in Galaxies , August 2012 , pp. 63
Copyright
Copyright © International Astronomical Union 2013

References

Taylor, A. R., Wallace, B. J., & Goss, W. M., 1992, AJ, 103, 931Google Scholar
Xu, J. L. & Wang, J. J. 2012, A&A, 543, 24Google Scholar