Limits on the presence of planets in systems with debris discs: HD 92945 and HD 107146

[en] Recent observations of resolved cold debris discs at tens of au have revealed that gaps could be a common feature in these Kuiper-belt analogues. Such gaps could be evidence for the presence of planets within the gaps or closer in near the edges of the disc. We present SPHERE observations of HD 92945 and HD 107146, two systems with detected gaps. We constrained the mass of possible companions responsible for the gap to 1-2 MJup for planets located inside the gap and to less than 5 MJup for separations down to 20 au from the host star. These limits allow us to exclude some of the possible configurations of the planetary systems proposed to explain the shape of the discs around these two stars. In order to put tighter limits on the mass at very short separations from the star, where direct-imaging data are less effective, we also combined our data with astrometric measurements from Hipparcos and Gaia and radial-velocity measurements. We were able to limit the separation and the mass of the companion potentially responsible for the proper-motion anomaly of HD 107146 to values of 2-7 au and 2-5 MJup, respectively. © 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.

Disciplines :

Space science, astronomy & astrophysics

Author, co-author :

Mesa, D.; INAF-Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padova, I-35122, Italy

Marino, S.; Max Planck Institute for Astronomy, Königstuhl 17, Heidelberg, D-69117, Germany, Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB3 0HA, United Kingdom

Bonavita, M.; INAF-Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padova, I-35122, Italy, Supa, Institute for Astronomy, University of Edinburgh, Blackford Hill, Edinburgh, EH9 3HJ, United Kingdom, Centre for Exoplanet Science, University of Edinburgh, Edinburgh, EH9 3HJ, United Kingdom

Lazzoni, C.; INAF-Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padova, I-35122, Italy, Dipartimento di Fisica A Astronomia 'G. Galilei', Universit'a di Padova, Via Marzolo, 8, Padova, I-35121, Italy

Fontanive, C.; INAF-Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padova, I-35122, Italy, Supa, Institute for Astronomy, University of Edinburgh, Blackford Hill, Edinburgh, EH9 3HJ, United Kingdom, Center for Space and Habitability, University of Bern, Gesellschaftsstrasse 6, Bern, CH-3012, Switzerland

Pérez, S.; Universidad de Santiago de Chile, Estacion Central, Av. Libertador Bernardo O'Higgins 3363, Santiago, Chile

D'Orazi, V.; INAF-Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padova, I-35122, Italy, School of Physics and Astronomy, Monash University, Clayton Campus, VIC 3800, Australia

Desidera, S.; INAF-Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padova, I-35122, Italy

Gratton, R.; INAF-Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padova, I-35122, Italy

Engler, N.; Eth Zurich, Institute for Particle Physics and Astrophysics, Wolfgang-Pauli-Strasse 27, Zurich, CH-8093, Switzerland

More authors (31 more)

Language :

English

Title :

Limits on the presence of planets in systems with debris discs: HD 92945 and HD 107146

Publication date :

2021

Journal title :

Monthly Notices of the Royal Astronomical Society

ISSN :

0035-8711

eISSN :

1365-2966

Publisher :

Oxford University Press, Oxford, United Kingdom

Volume :

503

Issue :

Pages :

1276-1289

Available on ORBi :

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