A dataset provided by the European Space Agency

Name OT2_gkennedy_2
Title Debris Disks as a Tracer of Star and Planet Formation in Binaries
URL

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DOI https://doi.org/10.5270/esa-4oydc6e
Author European Space Agency
Description We propose to observe nearby binary star systems to discover and characterise
circumbinary debris disks. With these data we will study the effects of cluster evolution
and long term stability on planet formation. The primary goal is to resolve disks, which
allows an analysis of the binary and disk orbital planes and leads to conclusions about
the formation and stability of the system. The secondary goal is to test whether dust
resides in unstable regions, which could be the result of a dynamical instability induced
by perturbations from the binary. Both goals focus on the dynamics of circumbinary
debris, and provide information on planet formation and survival in binary systems.
Publication A statistically significant lack of debris discs in medium separation binary systems . Yelverton Ben et al. . Monthly Notices of the Royal Astronomical Society . null . null . 2019MNRAS.488.3588Y ,
Instrument PACS_PacsPhoto_largeScan
Temporal Coverage 2012-01-12T11:52:04Z/2013-03-13T18:59:26Z
Version SPG v14.2.0
Mission Description Herschel was launched on 14 May 2009! It is the fourth 'cornerstone' mission in the ESA science programme. With a 3.5 m Cassegrain telescope it is the largest space telescope ever launched. It is performing photometry and spectroscopy in approximately the 55-671 µm range, bridging the gap between earlier infrared space missions and groundbased facilities.
Creator Contact https://support.cosmos.esa.int/h®erschel/
Date Published 2013-09-13T18:52:01Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013, Debris Disks As A Tracer Of Star And Planet Formation In Binaries, SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-4oydc6e