A dataset provided by the European Space Agency

Name OT2_mhaynes_2
Title Dust in the HIghMass Galaxies
URL

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DOI https://doi.org/10.5270/esa-fk77m7g
Author haynes, m.
Description We propose to obtain the PACS and SPIRE scan maps of a sample of 34 exceptionally gas-rich galaxies extracted from the ALFALFA extragalactic HI survey. These very HIgh HI mass (HIghMass) galaxies have HI masses > 10^10 Msun and are also very gas-rich for their stellar masses; 17/34 have M_HI>M_star. Are they in an arrested stage of evolution or do their huge HI disks, evident in our HI synthesis maps, result from recent baryon accretion? In combination with the HI synthesis maps (EVLA, GMRT, WSRT), GALEX UV, Halpha, optical broadband and CO studies, FIR/submm maps will cover a critical wavelength range of the dust emission spectral energy distribution and will allow us to determine the dust masses, temperatures and grain size distributions so that we can explore the interplay between the dust, stellar, gas and dark matter components within each galaxy and identify the dust variation trends within the HIghMass sample. In particular, Herschel observations will help us to (1) explore the unique dust behavior in the HIghMass galaxies and map the extent of the cold dust disk; (2) test the origin and evolutionary stage of them and infer molecular masses via the dust to gas ratio; (3) probe the dust-obscured star formation and study the dust heating mechanisms in their extended massive HI disks. Identified first as a class only by ALFALFA, the HIghMass galaxies represent the local counterparts of the populations which are likely to dominate future studies of HI at higher redshift with the Square Kilometer Array.
Publication
Instrument PACS_PacsPhoto_largeScan, SPIRE_SpirePhoto_small
Temporal Coverage 2012-06-08T19:49:42Z/2013-01-20T06:44:39Z
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 2013-07-20T06:39:32Z
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, haynes et al., 2013, 'Dust in the HIghMass Galaxies', SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-fk77m7g