A dataset provided by the European Space Agency

Name DDT_gkennedy_3
Title HIP 80946: A rare warm debris disk?


DOI 10.5270/esa-illqjdc
Author kennedy, g.
Description We propose to observe a nearby candidate warm dust system, HIP 89046, that we have recently identified with WISE. Such debris disk systems are extremely rare, and therefore characterising each individual is extremely important to understand their origin and evolution. This object shows mid-IR emission from several instruments that is most likely associated with the star. There is also significant far-IR emission, which AKARI-FIS suggests is associated with a nearby object rather than HIP 89046, but may mask emission from HIP 89046 itself. There is therefore an ambiguity as to whether HIP 89046 is a protoplanetary disk, or a bona fide warm dust source. These observations will resolve this ambiguity, and possibly result in confirmation of a new record holder as the "dustiest" warm debris disk.
Publication Evolution from protoplanetary to debris discs: the transition disc around HD 166191 . Kennedy G. M. et al. . Monthly Notices of the Royal Astronomical Society, Volume 438, Issue 4, p.3299-3309 . 438 . 10.1093\/mnras\/stt2435 . 2014MNRAS.438.3299K ,
Instrument PACS_PacsPhoto_largeScan
Temporal Coverage 2013-03-17T16:28:45Z/2013-03-17T16:47:21Z
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 ┬Ám range, bridging the gap between earlier infrared space missions and groundbased facilities.
Creator Contact https://support.cosmos.esa.int/herschel/
Date Published 2013-09-17T16:38:36Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-09-17T16:38:36Z, DDT_gkennedy_3, SPG v14.2.0. https://doi.org/10.5270/esa-illqjdc