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 European Space Agency
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 . Fernández-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 ,
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
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013, Heating The Cool Gas Filaments In Ngc 1275., SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-zseh2jj