A dataset provided by the European Space Agency

Name SDP_cwilso01_3
Title Physical Processes in the Interstellar Medium of Very Nearby Galaxies


DOI 10.5270/esa-q83sxpo
Author wilson, c.
Description We propose to use the SPIRE and PACS instruments on Herschel to measure the emission spectrum from dust as well as important cooling lines from the gaseous interstellar medium in sample of 13 very nearby galaxies (M51, M81, NGC2403, NGC891, M83, M82, Arp220, NGC4038-39, NGC1068, NGC4151, CenA, NGC4125, and NGC205). These galaxies have been chosen to probe as wide a region in galaxy parameter space as possible while maximizing the achievable spatial resolution and are already well-studied from X-ray and optical through to radio wavelengths. The far-infrared and submillimeter wavelengths probed by Herschel are absolutely crucial for understanding the physical processes and properties of the interstellar medium,the interplay between star formation and the interstellar medium in galaxies, and how they may depend on the wider galaxian environment.
Publication DustPedia: Multiwavelength photometry and imagery of 875 nearby galaxies in 42 ultraviolet-microwave bands . Clark C. J. R. et al. . Astronomy & Astrophysics, Volume 609, id.A37, 30 pp. . 609 . 10.1051\/0004-6361\/201731419 . 2018A&A...609A..37C ,
FIR colours and SEDs of nearby galaxies observed with Herschel . Boselli A. et al. . Astronomy and Astrophysics, Volume 518, id.L61, 5 pp. . 518 . 10.1051\/0004-6361\/201014534 . 2010A&A...518L..61B ,
The evolving far-IR galaxy luminosity function and dust-obscured star formation rate density out to z≃5. . Koprowski M. P. et al. . Monthly Notices of the Royal Astronomical Society, Volume 471, Issue 4, p.4155-4169 . 471 . 10.1093\/mnras\/stx1843 . 2017MNRAS.471.4155K ,
Variations of the ISM Compactness Across the Main Sequence of Star Forming Galaxies: Observations and Simulations . Martínez-Galarza J. R. et al. . The Astrophysical Journal, Volume 817, Issue 1, article id. 76, 18 pp. (2016). . 817 . 10.3847\/0004-637X\/817\/1\/76 . 2016ApJ...817...76M ,
Simulated Galaxy Interactions as Probes of Merger Spectral Energy Distributions . Lanz Lauranne et al. . The Astrophysical Journal, Volume 785, Issue 1, article id. 39, 20 pp. (2014). . 785 . 10.1088\/0004-637X\/785\/1\/39 . 2014ApJ...785...39L ,
Dust emissivity and absorption cross section in DustPedia late-type galaxies . Bianchi S. et al. . Astronomy and Astrophysics . null . null . 2019A&A...631A.102B ,
SPIRE imaging of M 82: Cool dust in the wind and tidal streams . Roussel H. et al. . Astronomy and Astrophysics, V...
Instrument SPIRE_SpireSpectrometer_, PACS_PacsPhoto_largeScan, SPIRE_SpirePhoto_large
Temporal Coverage 2009-10-06T19:13:41Z/2010-04-05T15:47:04Z
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/herschel/
Date Published 2010-10-06T19:13:41Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2010-10-06T19:13:41Z, SDP_cwilso01_3, SPG v14.2.0. https://doi.org/10.5270/esa-q83sxpo