A dataset provided by the European Space Agency

Name OT2_kstape01_1
Title The Final Four: Completing Herschel.s Imaging Legacy for Key Debris Disk Systems
URL

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DOI https://doi.org/10.5270/esa-r7w039d
Author stapelfeldt, k.
Description Debris disks are the signposts of planetary systems: collisions among asteroidal and cometary parent bodies maintain the observed dust population against losses to radiation pressure and P-R drag. While hundreds of debris disks are known fromfar-IR excecss emission around main sequence stars, the best-understood systems are the virgul20 that are spatially resolved.Disk images establish the size scale of an exoplanetary system.They can reveal central holes, rings, gaps, warps, and asymmetriesin the dust distribution which indicate the presence of planetaryperturbers. Disk images at different wavelengths are sensitive to dust grains of different sizes, and thus provide a way to trace dusttransport and segregation processes. In spring 2011 we discovered large new debris disk in HSTcoronagraphic images. The new system is an eccentric ring with a sharp inner edge and cleared central zone, and thus is remarkablysimilar to the classic Fomalhaut debris ring. Spitzer only detectedthe system at a single wavelength. We propose PACS and SPIRE imaging photometry to fully establish the spatial and spectralproperties of this new debris system, and of three otherHST-detected debris disks that lack Herschel measurements.Simultaneous modeling of the far-IR images, SEDs, and HST imagesof these disk will provide important constraints on the physicalproperties and dynamical state of their constituent dust.Our small program will complete Herschel.s legacy dataset forthe key subsample of bright disks that are detected in scacttered light,
Publication
  • Pursuing the Planet-Debris Disk Connection: Analysis of Upper Limits from the Anglo-Australian Planet Search | Wittenmyer Robert A. et al. | The Astronomical Journal Volume 149 Issue 2 article id. 86 7 pp. (2015). | 149 | 10.1088\\/0004-6256\\/149\\/2\\/86 | 2015AJ....149...86W | http://adsabs.harvard.edu/abs/2015AJ....149...86W
  • A search for trends in spatially resolved debris discs at far-infrared wavelengths | Marshall J. P. et al. | Monthly Notices of the Royal Astronomical Society | null | null | 2021MNRAS.501.6168M |
  • From Scattered-light to Millimeter Emission: A Comprehensive View of the Gigayear-old System of HD 202628 and its Eccentric Debris Ring | Faramaz Virginie et al. | The Astronomical Journal | null | null | 2019AJ....158..162F |
Instrument PACS_PacsPhoto_largeScan, SPIRE_SpirePhoto_small
Temporal Coverage 2012-03-22T03:49:52Z/2012-12-12T17:42:09Z
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 2013-06-12T17:28:09Z
Keywords Herschel, HSC, submillimetre, far-infrared, HIFI, PACS, SPIRE
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, stapelfeldt et al., 2013, 'The Final Four: Completing Herschel.s Imaging Legacy for Key Debris Disk Systems', SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-r7w039d