A dataset provided by the European Space Agency

Name OT2_roonk_1
Title Heating the cool gas filaments in NGC 1275.
URL

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342248350&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342248360&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342248361&instrument_name=PACS&product_level=LEVEL0&compress=true
DOI https://doi.org/10.5270/esa-zseh2jj
Author oonk, r.
Description We propose PACS CII, OI and NII spectra to determine the source of heating for the cool (20-300 K) gas in an isolated, quiescent gas filament in the Brightest Cluster Galaxy (BCG) NGC-1275, the brightest of all cluster cool-core galaxies. The heating mechanism of this cool gas in BCGs is not well understood, It is also crucial to understanding analogous negative feedback processes in star-forming galaxies at high redshift. In combination with our SPIRE spectroscopy, and other deep multi-wavelength measurements, the proposed observations will provide a unique data set that will allow us to develop a consistent physical picture of the processes that energize the filaments. NGC-1275 is the only cool-core BCG where we can separate the quiescent filaments from the nuclear region influenced by the AGN. This will allow us to directly compare the heating of cool gas in these filaments with that in the nuclear region.
Publication
  • Far-infrared Line Spectra of Active Galaxies from the Herschel/PACS Spectrometer: The Complete Database | Fernandez-Ontiveros Juan Antonio et al. | The Astrophysical Journal Supplement Series Volume 226 Issue 2 article id. 19 26 pp. (2016). | 226 | 10.3847\\/0067-0049\\/226\\/2\\/19 | 2016ApJS..226...19F | http://adsabs.harvard.edu/abs/2016ApJS..226...19F
Instrument PACS_PacsLineSpec_point
Temporal Coverage 2012-07-19T12:44:34Z/2012-07-20T10:43:09Z
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 2013-01-20T09:34:07Z
Keywords Herschel, HSC, submillimetre, far-infrared, HIFI, PACS, SPIRE
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, oonk et al., 2013, 'Heating the cool gas filaments in NGC 1275.', SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-zseh2jj