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Verfasst von:Musso Barcucci, Arianna [VerfasserIn]   i
 Launhardt, Ralf [VerfasserIn]   i
 Müller, André [VerfasserIn]   i
 Kennedy, Grant M. [VerfasserIn]   i
 Boekel, Roy van [VerfasserIn]   i
 Henning, Thomas [VerfasserIn]   i
 Ruh, Henrik Lukas [VerfasserIn]   i
 Marino, Sebastian [VerfasserIn]   i
 Pearce, Tim D. [VerfasserIn]   i
 Brems, Stefan S. [VerfasserIn]   i
 Ertel, Steve [VerfasserIn]   i
 Spalding, Eckhart A. [VerfasserIn]   i
Titel:LIStEN
Titelzusatz:L′ band imaging survey for exoplanets in the North
Verf.angabe:Arianna Musso Barcucci, Ralf Launhardt, André Müller, Grant M. Kennedy, Roy van Boekel, Thomas Henning, Henrik L. Ruh, Sebastian Marino, Tim D. Pearce, Stefan S. Brems, Steve Ertel, and Eckhart A. Spalding
E-Jahr:2021
Jahr:19 January 2021
Umfang:23 S.
Teil:volume:645
 year:2021
 elocationid:A88
 pages:1-23
 extent:23
Fussnoten:Gesehen am 07.04.2021
Titel Quelle:Enthalten in: Astronomy and astrophysics
Ort Quelle:Les Ulis : EDP Sciences, 1969
Jahr Quelle:2021
Band/Heft Quelle:645(2021), Artikel-ID A88, Seite 1-23
ISSN Quelle:1432-0746
Abstract:Context. Planetary systems and debris discs are natural by-products of the star formation process, and they affect each other. The direct imaging technique allows simultaneous imaging of both a companion and the circumstellar disc it resides in, and is thus a valuable tool to study companion-disc interactions. However, the number of systems in which a companion and a disc have been detected at the same time remains low. Aims. Our aim is to increase this sample, and to continue detecting and studying the population of giant planets in wide orbits. Methods. We carry out the L′ band Imaging Survey for Exoplanets in the North (LIStEN), which targeted 28 nearby stars: 24 are known to harbour a debris disc (DD) and the remaining 4 are protoplanetary disc-hosting stars. We aim to detect possible new companions, and study the interactions between the companion and their discs. Angular differential imaging observations were carried out in the L′ band at 3.8 μm using the LMIRCam instrument at the LBT, between October 2017 and April 2019. Results. No new companions were detected. We combined the derived mass detection limits with information on the disc, and on the proper motion of the host star, to constrain the presence of unseen planetary and low-mass stellar companion around the 24 disc-hosting stars in our survey. We find that 2 have an uncertain DD status and the remaining 22 have disc sizes compatible with self-stirring. Three targets show a proper motion anomaly (PMa) compatible with the presence of an unseen companion. Conclusions. Our achieved mass limits combined with the PMa analysis for HD 113337 support the presence of a second companion around the star, as suggested in previous RV studies. Our mass limits also help to tighten the constraints on the mass and semi-major axis of the unseen companions around HD 161868 and HD 8907.
DOI:doi:10.1051/0004-6361/202039541
URL:Bitte beachten Sie: Dies ist ein Bibliographieeintrag. Ein Volltextzugriff für Mitglieder der Universität besteht hier nur, falls für die entsprechende Zeitschrift/den entsprechenden Sammelband ein Abonnement besteht oder es sich um einen OpenAccess-Titel handelt.

Volltext ; Verlag: https://doi.org/10.1051/0004-6361/202039541
 Volltext: https://www.aanda.org/articles/aa/abs/2021/01/aa39541-20/aa39541-20.html
 DOI: https://doi.org/10.1051/0004-6361/202039541
Datenträger:Online-Ressource
Sprache:eng
K10plus-PPN:1753292107
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