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The super star cluster driven feedback in ESO338-IG04 and Haro 11

Published online by Cambridge University Press:  31 March 2017

A. Bik ,
G. Östlin ,
V. Menacho ,
A. Adamo ,
M. Hayes ,
J. Melinder  and
P. Amram
A. Bik
Affiliation:
Department of Astronomy, Oskar Klein Centre, Stockholm University, AlbaNova University Centre, 106 91 Stockholm, Sweden email: arjan.bik@astro.su.se
G. Östlin
Affiliation:
Department of Astronomy, Oskar Klein Centre, Stockholm University, AlbaNova University Centre, 106 91 Stockholm, Sweden email: arjan.bik@astro.su.se
V. Menacho
Affiliation:
Department of Astronomy, Oskar Klein Centre, Stockholm University, AlbaNova University Centre, 106 91 Stockholm, Sweden email: arjan.bik@astro.su.se
A. Adamo
Affiliation:
Department of Astronomy, Oskar Klein Centre, Stockholm University, AlbaNova University Centre, 106 91 Stockholm, Sweden email: arjan.bik@astro.su.se
M. Hayes
Affiliation:
Department of Astronomy, Oskar Klein Centre, Stockholm University, AlbaNova University Centre, 106 91 Stockholm, Sweden email: arjan.bik@astro.su.se
J. Melinder
Affiliation:
Department of Astronomy, Oskar Klein Centre, Stockholm University, AlbaNova University Centre, 106 91 Stockholm, Sweden email: arjan.bik@astro.su.se
P. Amram
Affiliation:
Aix Marseille Université, CNRS, LAM (Laboratoire dAstrophysique de Marseille), 13388 Marseille, France
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Abstract

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The stellar content of young massive star clusters emit large amounts of Lyman continuum photons and inject momentum into the inter stellar medium (ISM) by the strong stellar winds of the most massive stars in the cluster. When the most massive stars explode as supernovae, large amounts of mechanical energy are injected in the ISM. A detailed study of the ISM around these massive cluster provides insights on the effect of cluster feedback.

We present high quality integral field spectroscopy taken with VLT/MUSE of two starburst galaxies: ESO 338-IG04 and Haro 11. Both galaxies contain a significant number of super star clusters. The MUSE data provide us with an unprecedented view of the state and kinematics of the ionized gas in the galaxy allowing us to study the effect of stellar feedback on small and large spatial scales. We present our recent results on studying the ISM state of these two galaxies. The data of both galaxies show that the mechanical and ionization feedback of the super star clusters in the galaxy modify the state and kinematics of the ISM substancially by creating highly ionized bubbles around the cluster, making the central part of the galaxy highly ionized. This shows that the HII regions around the individual clusters are density bounded, allowing the ionizing photons to escape and ionize the ISM further out.

Keywords

galaxies: starburstgalaxies: individual: ESO338-IG04Haro 11galaxies: ISMgalaxiesstar clusters
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S316: Formation, evolution, and survival of massive star clusters , August 2015 , pp. 44 - 49
Copyright
Copyright © International Astronomical Union 2017 

References

Adamo, A., Östlin, G. Zackrisson, E., et al. 2010, MNRAS, 407, 870 CrossRefGoogle Scholar
Adamo, A., Östlin, G., & Zackrisson, E. 2011, MNRAS, 417, 1904 CrossRefGoogle Scholar
Bacon, R., Accardo, M., Adjali, L., et al. 2010, SPIE Conf. Ser., 7735, 08 Google Scholar
Bik, A., Östlin, G., Hayes, M., Adamo, A., Melinder, J., & Amram, P. 2015, A&A, 576, L13 Google Scholar
Cappellari, M. & Copin, Y. 2003, MNRAS, 342, 345 CrossRefGoogle Scholar
Cormier, D., Lebouteiller, V., Madden, S. C., et al. 2012, A&A, 548, 20 Google Scholar
Diehl, S. & Statler, T. S. 2006, MNRAS, 368, 497 CrossRefGoogle Scholar
Hayes, M., Östlin, G., Mas-Hesse, J. M., et al. 2005, A&A, 438, 71 Google Scholar
Leitet, E., Bergvall, N., Piskunov, N., & Andersson, B.-G. 2011, A&A, 532, A107 Google Scholar
Leitet, E., Bergvall, N., Hayes, M., Linné, S., & Zackrisson, E. 2013, A&A, 553, A106 Google Scholar
Leitherer, C., Schaerer, D., Goldader, J. D., et al. 1999, ApJS, 123, 3 CrossRefGoogle Scholar
Osterbrock, D. E. 1989, Astrophysics of Gaseous Nebulae and Active Galactic Nuclei (Mill Valley: University Science Books)CrossRefGoogle Scholar
Östlin, G., Bergvall, N., & Rönnback, J. 1998, A&A, 335, 85 Google Scholar
Östlin, G., Marquart, T., Cumming, R. J., et al. 2015, A&A in press, ArXiv:1508.00541Google Scholar
Östlin, G., Zackrisson, E., Bergvall, N., & Rönnback, J. 2003, A&A, 408, 887 Google Scholar
Overzier, Roderik A., Heckman, Timothy M., Kauffmann, Guinevere et al. 2008, ApJ, 677, 37 CrossRefGoogle Scholar
Pellegrini, E. W., Oey, M. S., Winkler, P. F., et al. 2012, ApJ, 755, 40 CrossRefGoogle Scholar
Vader, J. P., Frogel, J. A., Terndrup, D. M., & Heisler, C. A. 1993, AJ, 106, 1743 CrossRefGoogle Scholar
Zastrow, J., Oey, M. S., Veilleux, S., McDonald, M., & Martin, C. L. 2011, ApJ, 741, L17 CrossRefGoogle Scholar
Zastrow, J., Oey, M. S., Veilleux, S., & McDonald, M. 2013, ApJ, 779, 76 CrossRefGoogle Scholar