A dataset provided by the European Space Agency

Name OT2_jmartinp_3
Title Molecular Ions in Galaxies. Tracing the diffuse molecular component
URL

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DOI https://doi.org/10.5270/esa-j1qcyxe
Author martin-pintado, j.
Description We propose to use HIFI to observe a complete set of molecular ions related tothe PDR-XDR-CRs chemistry toward seven galaxies covering all types ofactivities. We have selected the hydrides CH+, CH, OH, H2O+, HCl, OH+ andH3O+, and the high density tracers HCN, HCO+ and HNC suggested to beaffected by X-ray and shock induced chemistry. To covera wide range of nuclear activity we will observe three ULIRGs, Arp 220 (cold),NGC4418 (warm) and Mrk231, one LIRG, Arp 299A, the AGN NGC1068, and twostarbursts, M82 and M83.The high spectral resolution provided by HIFI will be fundamental to disentangle the complex line profiles (usually P Cygni) often observed in galaxies due to clouds observed along the line of sight with different velocities and large changes in the molecular abundances ratios. The H2O, OH+, H2O+ and H3O+ abundances and abundance ratios will be used to disentangle the CR/Xray and the PDR components in the galaxies.
Publication
    Instrument HIFI_HifiPoint_dbs
    Temporal Coverage 2012-02-02T22:33:59Z/2013-01-15T23:22:37Z
    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 2013-07-15T21:57:01Z
    Keywords Herschel, HSC, submillimetre, far-infrared, HIFI, PACS, SPIRE
    Publisher And Registrant European Space Agency
    Credit Guidelines European Space Agency, martin-pintado et al., 2013, 'Molecular Ions in Galaxies. Tracing the diffuse molecular component', SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-j1qcyxe