Herschel PACS and SPIRE Imaging of CW Leonis

Ladjal, D., Barlow, M., Groenewegen, M., Ueta, T., Blommaert, J. A. D. L., Cohen, M., Decin, L., De Meester, W., Exter, K., Gear, Walter Kieran ORCID: https://orcid.org/0000-0001-6789-6196, Gomez, Haley Louise ORCID: https://orcid.org/0000-0003-3398-0052, Hargrave, Peter Charles ORCID: https://orcid.org/0000-0002-3109-6629, Hugyen, R., Ivison, R. J., Jean, C., Kerschbaum, F., Leeks, S. J., Lim, T. L., Olofsson, G., Polehampton, E., Posch, T., Regibo, S., Royer, P., Sibthorpe, B., Swinyard, B. M., Vandenbussche, B., Waelkens, C., Wesson, R., Lebzelter, T. and Wing, R. F. 2010. Herschel PACS and SPIRE Imaging of CW Leonis. Presented at: Why Galaxies Care About AGB Stars II, Vienna, Austria, 16-20 August 2010. Published in: Kerschbaum, F., Lebzelter, T., Wing, R. F. and Klotz, D. eds. Proceedings of a Conference on Why Galaxies Care About AGB Stars II Shining Examples and Common Inhabitants, Vienna, Austria, 16-20 August 2010. Astronomical Society of the Pacific conference series , vol.445 (445) San Francisco, CA: Astronomical Society of the Pacific, p. 337.

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Abstract

Far-IR (FIR) images of the archetype carbon star CW Leo (IRC +10216) by the Herschel Space Observatory (Pilbratt et al. 2010) reveal an extended structure at about 11′ from the star which correlates with the UV structure seen by the GALaxy Evolution EXplorer Space Observatory (GALEX) (Sahai & Chronopoulos 2010). The UV emission is believed to be due to the shocked asymptotic giant branch (AGB) wind with the interstellar medium (ISM) (Sahai & Chronopoulos). We present our main results from the Herschel data on the wind–ISM interaction.

Item Type:	Conference or Workshop Item (Paper)
Date Type:	Publication
Status:	Published
Schools:	Physics and Astronomy
Subjects:	Q Science > QB Astronomy
Publisher:	Astronomical Society of the Pacific
ISBN:	9781583817704
Related URLs:	Publisher
Last Modified:	19 Oct 2022 10:35
URI:	https://orca.cardiff.ac.uk/id/eprint/24902

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