A dataset provided by the European Space Agency

Name OT2_mboquien_4
Title High resolution observations of the warm dust in M33
URL

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342247408&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342247409&instrument_name=PACS&product_level=LEVEL0&compress=true

DOI 10.5270/esa-eo9yayc
Author boquien, m.
Description We request 9.9 hours of observing time to map M33 at 70 micron. This project will enable a spatially-resolved investigation of HII regions in this galaxy, with the goal of determining changes 1) in the respective amount of PAH, stochastic and equilibrium dust emissions, in order to 2) constrain the radiation field and the properties of dust emission as a function of the evolutionary phase of the HII regions and across the disk of the galaxy. We will resolve the internal structure and physical properties of the HII regions down to ~24 pc (<6"), and construct spatially-resolved, pixel-based, UV-to-FIR SEDs. This proposal is a key complement to the HerM33es key project which mainly focuses on the mapping of major FIR cooling lines, with only a small fraction of the time dedicated to imaging from 100 micron to 500 micron (PACS and SPIRE).
Publication Millimeter and submillimeter excess emission in M 33 revealed by Planck and LABOCA . Hermelo I. et al. . Astronomy & Astrophysics, Volume 590, id.A56, 22 pp. . 590 . 10.1051\/0004-6361\/201525816 . 2016A&A...590A..56H ,
A high-resolution, dust-selected molecular cloud catalogue of M33, the Triangulum Galaxy . Williams Thomas G. et al. . Monthly Notices of the Royal Astronomical Society, Volume 483, Issue 4, p.5135-5149 . 483 . 10.1093\/mnras\/sty3437 . 2019MNRAS.483.5135W ,
The star formation law at GMC scales in M33, the Triangulum galaxy . Williams Thomas G. et al. . Monthly Notices of the Royal Astronomical Society, Volume 479, Issue 1, p.297-314 . 479 . 10.1093\/mnras\/sty1476 . 2018MNRAS.479..297W ,
Dust properties in H II regions in M 33 . Relaño M. et al. . Astronomy & Astrophysics, Volume 595, id.A43, 22 pp. . 595 . 10.1051\/0004-6361\/201628139 . 2016A&A...595A..43R ,
Finding η Car Analogs in Nearby Galaxies Using Spitzer. II. Identification of An Emerging Class of Extragalactic Self-Obscured Stars . Khan Rubab et al. . The Astrophysical Journal, Volume 799, Issue 2, article id. 187, 14 pp. (2015). . 799 . 10.1088\/0004-637X\/799\/2\/187 . 2015ApJ...799..187K ,
Spatially resolving the dust properties and submillimetre excess in M 33 . Relaño M. et al. . Astronomy & Astrophysics, Volume 613, id.A43, 19 pp. . 613 . 10.1051\/0004-6361\/201732347 . 2018A&A...613A..43R ,
Measuring star formation with resolved observations: the test case of M 33 . Boquien M. ...
Instrument PACS_PacsPhoto_largeScan
Temporal Coverage 2012-06-25T02:20:11Z/2012-06-25T12:12:14Z
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 2012-12-25T07:16:45Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2012-12-25T07:16:45Z, OT2_mboquien_4, SPG v14.2.0. https://doi.org/10.5270/esa-eo9yayc