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Results from the Herschel Key Program MESS

Groenewegen, M. A. T., Waelkens, C., Barlow, M. J., Kerschbaum, F., Garcia-Lario, P., Cernicharo, J., Blommaert, J. A. D. L., Bouwman, J., Cohen, M., Cox, N., Decin, L., Exter, K., Gear, Walter Kieran ORCID:, Gomez, Haley Louise ORCID:, Hargrave, Peter Charles ORCID:, Henning, Th., Hutsemekers, D., Ivison, R. J., Jorissen, A., Krause, O., Ladjal, D., Leeks, S. J., Lim, T. L., Matsuura, Mikako ORCID:, Naze, Y., Olofsson, G., Ottensamer, R., Polehampton, E., Posch, T., Rauw, G., Royer, P., Sibthorpe, B., Swinyard, B. M., Ueta, T., Vamvatira- Nakou, C., Vandenbussche, B., Van de Steene, G. C., Van Eck, S., Van Hoof, P. A. M., Van Winckel, H., Verdugo, E. and Wesson, R. 2011. Results from the Herschel Key Program MESS. Presented at: Why Galaxies Care About AGB Stars 2, Vienna, Austria, 16-20 August 2010. 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, pp. 567-575.

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MESS (Mass loss of Evolved StarS) is a Herschel Guaranteed Time Key Program that will image about 100, and do spectroscopy of about 50, post-main-sequence objects of all flavours: AGB stars, post-AGB stars, planetary nebulae, luminous blue variables, Wolf-Rayet stars, and supernova remnants. In this review the implementation and current status of MESS is outlined, and first results are presented.

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
Last Modified: 19 Oct 2022 10:41

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