HD169142 Seen with New Eyes

Bertrang, Gesa H. -M.; Avenhaus, H.; Casassus, S.; Montesinos, M.; Kirchschlager, F.; Perez, S.; Cieza, L.; Wolf, S.

Item

ITEM ACTIONSEXPORT

Add to Basket

Local TagsRelease HistoryDetailsSummary

Released

Proceedings

HD169142 Seen with New Eyes

MPS-Authors

Bertrang, Gesa H. -M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Avenhaus, H.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Casassus, S.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Montesinos, M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Kirchschlager, F.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Perez, S.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Cieza, L.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Wolf, S.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

External Resource

https://ui.adsabs.harvard.edu/abs/2018dmss.confE...5B
(Any fulltext)

Fulltext (restricted access)

There are currently no full texts shared for your IP range.

Fulltext (public)

There are no public fulltexts stored in PuRe

Supplementary Material (public)

There is no public supplementary material available

Citation

Bertrang, G.-H.-.-M., Avenhaus, H., Casassus, S., Montesinos, M., Kirchschlager, F., Perez, S., et al. (2018). HD169142 Seen with New Eyes.

Cite as: https://hdl.handle.net/21.11116/0000-0005-CEE8-E

Abstract

The circumstellar disk around the Herbig Ae/Be star HD169142 is a well- studied object which shows structures on multiple wavelength ranges. Moreover, HD169142 harbors the most promising proto-planet candidate. We present new SPHERE/ZIMPOL data which distinctly deviate from the established picture developed for this object. Based on these new observations as well as high-resolution ALMA observations and further archival data, we built a new model for this disk. These new eyes, namely SPHERE and ALMA, in combination with 3D radiative transfer simulations strongly indicate that we are witness to previously undetected planet-disk interactions in HD169142.