A dataset provided by the European Space Agency

Name KPOT_ckrame01_1
Title Herschel M33 extended survey (HERMES): star-formation interplay with the ISM
URL

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DOI https://doi.org/10.5270/esa-a12i4wy
Author kramer, c.
Description In the local universe, most of the observable matter is contained instellar objects shaping the morphology and dynamics of their parentgalaxy. In view of the dominance of stellar mass, a betterunderstanding of star formation and its consequences is mandatory andforms a central topic of contemporary astrophysical research. Thereexist a large number of high linear resolution studies related toindividual star forming regions of the Galaxy as well as of low linearresolution studies of external galaxies. For a complete view onto thephysical and chemical processes driving star formation and galacticevolution it is, however, essential to combine local conditionsaffecting individual star formation with properties only becomingapparent on global scales.The optimal target providing such a complete view is a galaxy that is actively forming stars, that is not seen edge-on (like our Galaxy), that has been studied at radio, optical and X-ray wavelengths, and that is sufficiently nearby to also permit studies on smallscales. For our carefully chosen template galaxy, we plan to use HIFI to obtain fully-sampled large-scale CII (and H2O) maps. PACS will add important interstellar cooling lines, OI, NII, NIII. And SPIRE & PACS will be used to map the dust spectralenergy distribution over the entire galaxy.Observing a deep, extended strip along the major axis of our template galaxy M33, will allow us to study the ionized, atomic, and molecular phases of the interstellar medium, its life cycle andthermal balance, tracing the formation of molecular clouds and of stars. Aside of insightsrelated to the local processes in the galaxy itself,the mapped source will set a standard, providing a basis for the interpretation of phenomena encountered in other targets of the Local Group and in more distant galaxies.
Publication
  • The Panchromatic Hubble Andromeda Treasury: Triangulum Extended Region (PHATTER). I. Ultraviolet to Infrared Photometry of 22 Million Stars in M33 | Williams Benjamin F. et al. | The Astrophysical Journal Supplement Series | null | null | 2021ApJS..253...53W |
  • Strong C+ Emission in Galaxies at z virgul 1-2: Evidence for Cold Flow Accretion Powered Star Formation in the Early Universe | Brisbin Drew et al. | The Astrophysical Journal Volume 799 Issue 1 article id. 13 18 pp. (2015). | 799 | 10.1088\\/0004-637X\\/799\\/1\\/13 | 2015ApJ...799...13B | http://adsabs.harvard.edu/abs/2015ApJ...799...13B
  • The Herschel M 33 extended survey (HerM33es): PACS spectroscopy of the star-forming region BCLMP 302 | Mookerjea B. et al. | Astronomy & Astrophysics Volume 532 id.A152 12 pp. | 532 | 10.1051\\/0004-6361\\/201116447 | 2011A&A...532A.152M | http://adsabs.harvard.edu/abs/2011A%26A...532A.152M
  • Velocity resolved C II spectroscopy of the center and the BCLMP 302 region of M 33 (HerM 33es) | Mookerjea B. et al. | Astronomy & Astrophysics Volume 586 id.A37 13 pp. | 586 | 10.1051\\/0004-6361\\/201527366 | 2016A&A...586A..37M | http://adsabs.harvard.edu/abs/2016A%26A...586A..37M
  • Early Science with the Large Millimeter Telescope: CO and C II Emission in the z = 4.3 AzTEC J095942.9+022938 (COSMOS AzTEC-1) | Yun Min S. et al. | Monthly Notices of the Royal Astronomical Society Volume 454 Issue 4 p.3485-3499 | 454 | 10.1093\\/mnras\\/stv1963 | 2015MNRAS.454.3485Y | http://adsabs.harvard.edu/abs/2015MNRAS.454.3485Y
  • APEX CO observations towards the photodissociation region of RCW 120 | Figueira M. et al. | Astronomy and Astrophysics | null | null | 2020A&A...639A..93F |
Instrument HIFI_HifiPoint_load, HIFI_HifiMapping_load-raster, SPIRE\/PACS parallel_SpirePacsParallel_, PACS_PacsLineSpec_large
Temporal Coverage 2010-01-07T11:39:27Z/2012-07-21T14:40:42Z
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 2013-01-21T06:00:41Z
Keywords Herschel, HSC, submillimetre, far-infrared, HIFI, PACS, SPIRE
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, kramer et al., 2013, 'Herschel M33 extended survey openParHERMESclosePar: star-formation interplay with the ISM', SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-a12i4wy