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 European Space Agency
Description
Dusty disks around hot (Teff > 100,000 K) white dwarfs are a new
phenomenon discovered by Spitzer. The origin of such a disk is still
in debate. We propose to obtain far-infrared photometry for 6 dusty
disks around hot WDs identified from our Spitzer 24 micron survey. The
Herschel far-infrared measurements will provide strong constraints on
the outer boundary of the disk and its total dust mass in the system,
crucial information necessary to differentiate the origin of the
disks.
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
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2012, Dusty Disks Around Hot White Dwarfs: Debris Disks Or Remnant Of Post-Agb Binary Disksquestionmark, SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-dc8tgst