A dataset provided by the European Space Agency

Name OT1_ksu_2
Title Dusty Disks around Hot White Dwarfs: Debris Disks or Remnant of post-AGB Binary Disks?
URL

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DOI https://doi.org/10.5270/esa-dc8tgst
Author su, k.
Description Dusty disks around hot (Teff > 100,000 K) white dwarfs are a newphenomenon discovered by Spitzer. The origin of such a disk is stillin debate. We propose to obtain far-infrared photometry for 6 dustydisks around hot WDs identified from our Spitzer 24 micron survey. TheHerschel far-infrared measurements will provide strong constraints onthe outer boundary of the disk and its total dust mass in the system,crucial information necessary to differentiate the origin of thedisks.
Publication
    Instrument PACS_PacsPhoto_largeScan, SPIRE_SpirePhoto_small
    Temporal Coverage 2011-06-11T16:48:21Z/2012-04-24T00:38:20Z
    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 2012-10-24T00:19:38Z
    Last Update 2025-01-24
    Keywords Herschel, HSC, submillimetre, far-infrared, HIFI, PACS, SPIRE
    Publisher And Registrant European Space Agency
    Credit Guidelines European Space Agency, su et al., 2012, 'Dusty Disks around Hot White Dwarfs: Debris Disks or Remnant of post-AGB Binary Disks?', SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-dc8tgst