A dataset provided by the European Space Agency

Name OT2_jhigdon_3
Title The Over-Cooked ISM of Starburst Ring Galaxies
URL

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http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342257775&instrument_name=PACS&product_level=LEVEL0&compress=true

DOI https://doi.org/10.5270/esa-lj0khe1
Author higdon, j.
Description Studies of evolved systems like AM0644-741 and Cartwheel find the ISM in the starburst rings to be overwhelmingly atomic despite conditions (e.g., pressure and ambient far-UV fields)clearly favoring a dominant molecular component. Moreover, thelocal molecular fraction anti-correlates with SFR/area, yielding unusually high star formation efficiencies (SFE) and a highlypeculiar star formation law. AM0644-741s starburst ringmoreover appears mostly stable gravitationally (Q = 2-6). We have argued that these all follow naturally from the ISMs >100 Myr confinement time in the ring, which amplifies the destructive effects of embedded OB stars and SNe, producing an over-cooked ISM, i.e., one characterized by small H2 clouds, and a large photo-dissociated HI background. Due to reduceddust columns, H2 is poorly traced by CO rotational lines, and weexpect a large dark molecular component in the ring. Wewill use PACS and SPIRE photometry with existing IRAC and MIPSdata to (1) construct infrared-submillimeter SEDs for the rings of AM0644-741 and Cartwheel to determine the total mass anddistribution of H2 by its dust emission following Israel (1996)and Leroy et al. (2009), (2) re-evaluate their peculiar SFE,non-Schmidt star formation laws, and gravitational stability.Not finding a large hidden H2 component would imply thatstar formation is triggered by other processes (e.g., collisions)at unusually high SFE.
Publication
    Instrument PACS_PacsPhoto_largeScan, SPIRE_SpirePhoto_small
    Temporal Coverage 2012-03-01T10:16:56Z/2012-12-25T23:31:21Z
    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 2013-06-25T23:02:02Z
    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, higdon et al., 2013, 'The Over-Cooked'' ISM of Starburst Ring Galaxies', SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-lj0khe1