A dataset provided by the European Space Agency

Name OT1_ckiss_1
Title Exploring the gaseous component of debris disks of high fractional luminosity :
a deep O I 63.2 micron survey with Herschel.
URL

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DOI https://doi.org/10.5270/esa-o9n2kjw
Author kiss, c.
Description Gas-rich primordial disks and tenuous gas-poor debris disks
are usually considered as two distinct evolutionary phases of
the circumstellar matter. However, there is a very small interesting
group of stars in our neighbourhood (49 Ceti, and our discovery
HD 21997), which may represent the missing link between these
phases as indicated by the unexpected presence of debris-like
dust content and measurable CO gas component. With the aim
of discovering and characterizing more of these spectacular
objects here we propose to obtain O I 63 micron observations
of a sample of carefully selected young (<50Myr) debris disks of
high fractional luminosity with Herschel/PACS. Our objectives are to
1) discover and determine the incidence of 49 Ceti-like gaseous
debris disks; 2) characterize disk structure; 3) determine the
timescale of gas dispersal; 4) perform a detailed investigation
of HD 21997. New discoveries would lead to the definition of
a new subclass of circumstellar disks, the gaseous debris disks.
We required 17.2h of Herschel time for the observations.
Publication
  • Herschel-PACS observations of far-IR lines in young stellar objects. I. OI and H2O at 63 mm | Riviere-Marichalar P. et al. | Astronomy & Astrophysics Volume 594 id.A59 25 pp. | 594 | 10.1051\\/0004-6361\\/201527829 | 2016A&A...594A..59R | http://adsabs.harvard.edu/abs/2016A%26A...594A..59R
Instrument PACS_PacsPhoto_largeScan, SPIRE_SpirePhoto_small, PACS_PacsLineSpec_point
Temporal Coverage 2011-01-11T11:22:13Z/2013-04-27T03:36:13Z
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 2013-10-27T03:31:37Z
Keywords Herschel, HSC, submillimetre, far-infrared, HIFI, PACS, SPIRE
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, kiss et al., 2013, 'Exploring the gaseous component of debris disks of high fractional luminosity :
a deep [O I] 63.2 micron survey with Herschel.', SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-o9n2kjw