A dataset provided by the European Space Agency

Name OT2_ptemi_4
Title Diffuse Dust Emission from Black Hole-driven Outflows in Halo-centered Massive Elliptical Galaxies
URL

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342270945&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342270945&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342270946&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342270946&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342271021&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342271021&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342271022&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342271022&instrument_name=PACS&product_level=LEVEL0&compress=true

DOI https://doi.org/10.5270/esa-pekywgk
Author temi, p.
Description Dust grains ejected into the hot interstellar gas in group-centeredelliptical (E) galaxies are destroyed by ion-grain collisions, butduring their short lifetime (10 Myrs) the grains emit sufficiently inthe far infrared (FIR) to be easily observable. Remarkably, againstthis background emission, observations with Spitzer discovered many Egalaxies with much stronger and spatially extended FIR emission fromcolder grains 5-10 kpc distant from the galaxy cores. Extended excesscold dust emission is interpreted as evidence of recentfeedback-generated AGN energy outbursts in these galaxies, visibleonly in the FIR, from buoyant gaseous outflows from the galaxy cores.With Spitzer a quasi-radial plume of AGN-heated gas is resolved inonly one galaxy, but marginally resolved in others. We requestHerschel observations of a small sample of these E galaxies to confirmthe existence of excess, spatially extended dust and to possiblyspatially resolve more quasi-radial buoyant dusty gaseous plumes.Based on a detailed analysis of Spitzer data, our sample for Herschelis chosen to maximize the likelihood of discovering new FIR evidenceof post-feedback events from massive galaxy-centered black holes.
Publication
  • Spectral Energy Distribution Mapping of Two Elliptical Galaxies on Sub-kpc Scales | Amblard A. et al. | The Astrophysical Journal Volume 834 Issue 1 article id. 20 14 pp. (2017). | 834 | 10.3847\\/1538-4357\\/834\\/1\\/20 | 2017ApJ...834...20A | http://adsabs.harvard.edu/abs/2017ApJ...834...20A
Instrument PACS_PacsPhoto_largeScan
Temporal Coverage 2013-04-26T19:00:51Z/2013-04-27T19:19:38Z
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 2013-10-27T18:30:01Z
Keywords Herschel, HSC, submillimetre, far-infrared, HIFI, PACS, SPIRE
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, temi et al., 2013, 'Diffuse Dust Emission from Black Hole-driven Outflows in Halo-centered Massive Elliptical Galaxies', SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-pekywgk