A dataset provided by the European Space Agency

Name OT2_jmartinp_4
Title The Galactic center as the laboratory to understand nuclear activity in galaxies (GC_JMP)
URL

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DOI https://doi.org/10.5270/esa-4d9ffhs
Author martin-pintado, j.
Description We propose to use the The Galactic center (GC) a local extragalactic laboratory tounderstand the chemistry and the heating mechanisms in nearby galactic nuclei. Thecentral 30 pc region around the black hole, Sgr A*, contains all the different typeof activity found in extragalactic nuclei, namely, massive stellar clusterscreating large photodissociation regions (PDR), shocks, molecular clouds irradiatedby strong X-rays (XDRs), and the site of Cosmic Rays (CRs) acceleration as shown byHESS. We plan to map this region with SPIRE in the high spectral resolution mode and with HIFI in selected molecular ions H$_3$O$^+$, OH$^+$, and H$_2$O$^+$ claimed totrace XDRs and/or CRs. This unique data set will provide the possibility to understandthe origin of the large column densities of this hydrides found in galactic nucleiwith different type of activity and the role of the PDR-XDR-CR chemistries in theirformation. The SPIRE data cubes will have a huge legacy value providing the full FIRinventory of the atomic and molecular gas across the central 50 pc of the Galaxy. Westress that only the combination of the high spectral resolution of HIFI and thespatial distribution provided the proposed mapping will have the possibility todistinguish which of the different components of the molecular gas along the line ofsight correspond to the ones associated with XDRs PDRs and eventually CRsacceleration sites.
Publication
  • Herschel water maps towards the vicinity of the black hole Sgr A* | Armijos-Abendano J. et al. | Astronomy and Astrophysics | null | null | 2019A&A...624A.112A |
Instrument SPIRE_SpireSpectrometer_, HIFI_HifiPoint_pos, HIFI_HifiMapping_load-raster, HIFI_HifiMapping_fly
Temporal Coverage 2012-09-06T10:42:43Z/2012-10-17T23:04:22Z
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 2013-04-17T20:50:57Z
Last Update 2026-03-02
Keywords Herschel Space Observatory data, ESA Herschel mission dataset, far-infrared astronomy observations, submillimeter astronomy data, infrared space telescope observations, PACS photometer data, PACS spectrometer data, SPIRE photometer data, SPIRE Fourier transform spectrometer data, HIFI heterodyne spectroscopy data, far-infrared spectroscopy dataset, submillimeter spectral line observations, cold universe observations dataset, star formation infrared data, molecular cloud far-infrared observations, interstellar medium spectroscopy data, protoplanetary disk infrared observations, galaxy evolution far-infrared data, dust emission submillimeter observations, cosmic infrared background measurements, extragalactic infrared survey data, calibrated level 2 data products, FITS files astronomy, spectral cubes far-infrared, flux-calibrated maps, continuum photometry data, spectral energy distribution measurements, ESA Herschel Science Archive data
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, martin-pintado et al., 2013, 'The Galactic center as the laboratory to understand nuclear activity in galaxies (GC_JMP)', SPG v14.1.0, European Space Agency, https://doi.org/10.5270/esa-4d9ffhs