A dataset provided by the European Space Agency

Name GT2_ncox_1
Title Faint Extended Dust Envelopes of Young Planetary Nebulae
URL

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342237204&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342237205&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342237206&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342237207&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342241507&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342241508&instrument_name=PACS&product_level=LEVEL0&compress=true

DOI https://doi.org/10.5270/esa-88gpetg
Author cox, n.
Description We propose to trace the distribution of cold dust in the extended envelopes of aselected sample of young Planetary Nebulae (PNe). Information on the mass-loss andoverall envelope ejection process of Asymptotic Giant Branch (AGB) stars isimprinted in the morphology of the extended dust shells formed throughout the AGBphase. In particular the origin of asymmetrical PN shapes and their relation to spherical mass-loss presumed to occur on the AGB phase can be illuminated upon. Wepropose to use PACS to follow-up on AKARI/FIS observations of young PNe to studytheir mass-loss history. Only Herschels unprecedented spatial resolution andsensitivity in the far-IR can detect the faint extended cold dust emission in theseobjects.
Publication
    Instrument PACS_PacsPhoto_largeScan
    Temporal Coverage 2012-01-12T02:49:44Z/2012-03-16T06:30:42Z
    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 2012-09-16T06:01:36Z
    Last Update 2026-03-02
    Keywords Herschel Space Observatory data, ESA Herschel mission dataset, far-infrared astronomy observations, submillimeter astronomy data, infrared space telescope observations, PACS photometer data, PACS spectrometer data, SPIRE photometer data, SPIRE Fourier transform spectrometer data, HIFI heterodyne spectroscopy data, far-infrared spectroscopy dataset, submillimeter spectral line observations, cold universe observations dataset, star formation infrared data, molecular cloud far-infrared observations, interstellar medium spectroscopy data, protoplanetary disk infrared observations, galaxy evolution far-infrared data, dust emission submillimeter observations, cosmic infrared background measurements, extragalactic infrared survey data, calibrated level 2 data products, FITS files astronomy, spectral cubes far-infrared, flux-calibrated maps, continuum photometry data, spectral energy distribution measurements, ESA Herschel Science Archive data
    Publisher And Registrant European Space Agency
    Credit Guidelines European Space Agency, cox et al., 2012, 'Faint Extended Dust Envelopes of Young Planetary Nebulae', SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-88gpetg