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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S299(8), p. 208-209, 2013

DOI: 10.1017/s174392131300834x

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The multiple spirals in the disk of HD100546

Journal article published in 2013 by A. Boccaletti, A.-M. Lagrange, E. Pantin, J.-C. Augereau ORCID, S. P. Quanz, H. Meheut
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Data provided by SHERPA/RoMEO

Abstract

AbstractWe report the detection of multi-armed spirals in the environment of HD 100546 using NICI at Gemini South in the Ks band. These data feature a better angular resolution and higher contrast than previous HST images, which allows to resolve the former known spiral into a multiple pattern. An analytic model with a gravitational perturber is used to fit the spiral pattern. We derived limit of detections which set constraints on the discovered forming planet.

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