Decin, L. ; Royer, P. ; Cox, N. L. J. ; Vandenbussche, B. ; Ottensamer, R. ; Blommaert, J. A. D. L. ; Groenewegen, M. A. T. ; Barlow, M. J. ; Lim, T. ; Kerschbaum, F. ; Posch, T. ; Waelkens, C.

published in Astronomy and Astrophysics, 534, pp. A1 (2011)

Abstract: We present new Herschel/PACS images at 70, 100, and 160 µm of the well-known, nearby, carbon-rich asymptotic giant branch star IRC+10216 revealing multiple dust shells in its circumstellar envelope. For the first time, dust shells (or arcs) are detected until 320''. The almost spherical shells are non-concentric and have an angular extent between ~40° and ~200°. The shells have a typical width of 5''-8'', and the shell separation varies in the range of ~10''-35'', corresponding to ~500 -1 700 yr. Local density variations within one arc are visible. The shell/intershell density contrast is typically ~4, and the arcs contain some 50% more dust mass than the smooth envelope. The observed (nested) arcs record the mass-loss history over the past 16 000 yr, but Rayleigh-Taylor and Kelvin-Helmholtz instabilities in the turbulent astropause and astrosheath will erase any signature of the mass-loss history for at least the first 200 000 yr of mass loss. Accounting for the bowshock structure, the envelope mass around IRC+10216 contains >2 M? of gas and dust mass. It is argued that the origin of the shells is related to non-isotropic mass-loss events and clumpy dust formation. Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.

DOI: 10.1051/0004-6361/201117360
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