A dataset provided by the European Space Agency

Name OT1_wjaffe_1
Title Keeping the cool gas in galaxy clusters warm.
URL

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342249055&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342250527&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342250528&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342250529&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342250530&instrument_name=SPIRE&product_level=LEVEL0&compress=true
DOI https://doi.org/10.5270/esa-kyz0qd3
Author jaffe, w.
Description We propose SPIRE FTS spectra to determine the source of heating of the cool/warm (100-300 K) gas in the Brightest Cluster Galaxy NGC-1275, the brightest of all cluster cool-core galaxies. The heating mechanism in BCGs is unknown and crucial to understandinganalogous negative feedback processes in star-forming galaxiesat high redshift. Our current mm-CO, PACS, nearIR and optical dataon this cluster indicate that the SPIRE measurements will detectmany CO lines and possibly H2O+ and OH+ lines that willdetermine the temperature, and density of the most importantcomponent of this warm gas. The ratios of the CO lines, andthe presence or absence of the ionized lines, and thedependence of these lines with distance from the central AGN shouldallow us to choose between the several possible heatingand excitation mechanisms: soft X-rays, cosmic ray ionization,and C- and J- shocks from AGN induced turbulence.
Publication
  • On the far-infrared metallicity diagnostics: applications to high-redshift galaxies | Rigopoulou D. et al. | Monthly Notices of the Royal Astronomical Society Volume 473 Issue 1 p.20-29 | 473 | 10.1093/mnras/stx2311 | 2018MNRAS.473...20R | http://adsabs.harvard.edu/abs/2018MNRAS.473...20R
  • The Herschel SPIRE Fourier Transform Spectrometer Spectral Feature Finder - II. Estimating radial velocity of SPIRE spectral observation sources | Scott Jeremy P. et al. | Monthly Notices of the Royal Astronomical Society | null | null | 2020MNRAS.496.4894S |
  • Neutral carbon and CO in 76 (U)LIRGs and starburst galaxy centers. A method to determine molecular gas properties in luminous galaxies | Israel F. P. et al. | Astronomy & Astrophysics Volume 578 id.A95 16 pp. | 578 | 10.1051/0004-6361/201425175 | 2015A&A...578A..95I | http://adsabs.harvard.edu/abs/2015A%26A...578A..95I
  • AGN impact on the molecular gas in galactic centres as probed by CO lines | Esposito Federico et al. | Monthly Notices of the Royal Astronomical Society | null | null | 2022MNRAS.512..686E |
Instrument SPIRE_SpireSpectrometer_
Temporal Coverage 2012-08-04T05:14:21Z/2012-09-03T13:44:28Z
Version SPG v14.1.0
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 2013-03-03T09:37:16Z
Last Update 2025-01-24
Keywords Herschel, HSC, submillimetre, far-infrared, HIFI, PACS, SPIRE
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, jaffe et al., 2013, 'Keeping the cool gas in galaxy clusters warm.', SPG v14.1.0, European Space Agency, https://doi.org/10.5270/esa-kyz0qd3