Near-infrared scattered light properties of the HR 4796 A dust ring

Near-infrared scattered light properties of the HR 4796 A dust ring

Context. HR4796A is surrounded by a debris disc, observed in scattered light as an inclined ring with a high surface brightness. Past observations have raised several questions. First, a strong brightness asymmetry detected in polarised reflected light has recently challenged our understanding of sc...

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Bibliographic Details
Main Authors: Milli, J., Vigan, A., Mouillet, D., Lagrange, A.-M., Augereau, J.-C., Pinte, C., Mawet, D., Schmid, H. M., Boccaletti, A., Matrà, L., Kral, Q., Ertel, S., Chauvin, G., Bazzon, A., Ménard, F., Beuzit, J.-L., Thalmann, C., Dominik, C., Feldt, M., Henning, T., Min, M., Girard, J. H., Galicher, R., Bonnefoy, M., Fusco, T., de Boer, J., Janson, M., Maire, A.-L., Mesa, D., Schlieder, J. E.
Other Authors: Univ Arizona, Steward Observ
Language:en
Published: EDP SCIENCES S A 2017
Subjects:
instrumentation: high angular resolution
planet-disk interactions
planets and satellites: detection
scattering
planetary systems
Online Access:http://hdl.handle.net/10150/623201
http://arizona.openrepository.com/arizona/handle/10150/623201

Internet

http://hdl.handle.net/10150/623201
http://arizona.openrepository.com/arizona/handle/10150/623201

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