XMM-Newton view of the N 206 superbubble in the Large Magellanic Cloud

Kavanagh P, Sasaki M, Points S (2012)

Publication Status: Published

Publication Type: Journal article

Publication year: 2012

Journal

Astronomy & Astrophysics EDP Sciences

Publisher: EDP SCIENCES S A

Book Volume: 547

DOI: 10.1051/0004-6361/201219532

Abstract

Conclusions. Using the high-sensitivity X-ray data from XMM-Newton and optical data from the Magellanic Cloud Emission Line Survey has allowed us to better understand the physical properties of the N 206 superbubble and address some key questions of superbubble evolution.

Authors with CRIS profile

Manami Sasaki Professur für Multiwellenlängenastronomie

Involved external institutions

Cerro Tololo Inter-American Observatory (CTIO) CL Chile (CL) Dublin Institute for Advanced Studies (DIAS) IE Ireland (IE)

How to cite

APA:

Kavanagh, P., Sasaki, M., & Points, S. (2012). XMM-Newton view of the N 206 superbubble in the Large Magellanic Cloud. Astronomy & Astrophysics, 547. https://doi.org/10.1051/0004-6361/201219532

MLA:

Kavanagh, Patrick, Manami Sasaki, and Sean Points. "XMM-Newton view of the N 206 superbubble in the Large Magellanic Cloud." Astronomy & Astrophysics 547 (2012).

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