A dataset provided by the European Space Agency

Name OT2_ementuch_1
Title Dust temperatures in nearby turbulent disk galaxies: evidence for nearby cold flow gas accretion?
URL

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DOI 10.5270/esa-8t8lhsf
Author mentuch cooper, e.
Description We propose a survey of PACS (at 70 and 160 micron) and SPIRE (at 250, 350 and 500 micron) imaging of a sample of 31 of the most turbulent and intensely star forming galaxies in the local universe to measure their characteristic dust temperatures, dust masses and total infrared luminosities. These galaxies, selected from the all sky SDSS survey as the most H(alpha) bright galaxies in the nearby universe, have high velocity dispersions but show signs of ordered disk rotation (Green et al 2010) and as a consequence have more similarities to high-redshift turbulent disk galaxies than dynamically-relaxed galaxies common to the local universe. But are these truly low redshift analogues of turbulent rotating disks or are they currently undergoing a starburst episode? While both galaxy types are expected to be bright in the infrared, the former would have a much lower characteristic dust temperature that can efficiently be measured with Herschel due to the proximity (0.06
Publication
Instrument PACS_PacsPhoto_largeScan, SPIRE_SpirePhoto_small
Temporal Coverage 2012-06-10T22:29:02Z/2013-04-17T09:26:20Z
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 ┬Ám range, bridging the gap between earlier infrared space missions and groundbased facilities.
Creator Contact https://support.cosmos.esa.int/herschel/
Date Published 2013-10-17T09:23:31Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-10-17T09:23:31Z, OT2_ementuch_1, SPG v14.2.0. https://doi.org/10.5270/esa-8t8lhsf