A dataset provided by the European Space Agency

Name KPGT_cceccare_1
Title HIFI Spectral Surveys of Star Forming Regions
URL

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DOI 10.5270/esa-jhvlcfb
Author ceccarelli, c.
Description Study of the molecular content of regions far beyond our Solar System has advanced enormously during the last few decades, from the first detections of diatomic molecules to the discovery of polyatomic, complex organic molecules. Nowadays, one major goal of Astrochemistry is to have the most accurate census of the molecular content (and complexity) in Star Forming Regions (SFRs). In the era of the molecular content census, unbiased spectral surveys in the radio to Infrared of SFRs have become a fundamental and necessary tool in modern astrochemistry research. In this context, the frequency range covered by HSO-HIFI, 500-2000 GHz, is of particular importance. It is in this frequency range that light molecules have their ground and low energy transitions, whereas heavier molecules have higher energy transitions. The latter are excited in the warm gas, whereas the former probe the gas at low temperatures as well. It is therefore in the HIFI frequency range that the major gas coolants (notably H _2 O) and some key components of the chemical composition of SFRs emit. We propose to obtain Spectral Surveys in the HSO-HIFI range of a representative sample of SFRs. To have a meaningful coverage of the different evolutionary stages and different masses requires a large amount of time, about 300 hrs. The proposed observations will provide a large dataset of uttermost interest for the entire astronomical community, and, particularly for the study of star formation processes and of the influence of chemistry on star and planet formation. These two basic aspects, a large requested observing time and an output of high archival value, make the present proposal suitable for a HSO Key Program.
Publication Ortho-to-para ratio of interstellar heavy water . Vastel C. et al. . Astronomy and Astrophysics, Volume 521, id.L31, 5 pp. . 521 . 10.1051\/0004-6361\/201015101 . 2010A&A...521L..31V ,
A study of deuterated water in the low-mass protostar IRAS 16293-2422 . Coutens A. et al. . Astronomy & Astrophysics, Volume 539, id.A132, 12 pp. . 539 . 10.1051\/0004-6361\/201117627 . 2012A&A...539A.132C ,
Exploring the Origins of Earth’s Nitrogen: Astronomical Observations of Nitrogen-bearing Organics in Protostellar Environments . Rice Thomas S. et al. . The Astrophysical Journal, Volume 866, Issue 2, article id. 156, 16 pp. (2018). . 866 . 10.3847\/1538-4357\/aadfdb . 2018ApJ...866..156R ,
Heavy water stratification in a low-mass protostar . Coutens A. et al. . Astronomy & Astrophysics, Volume 553, id.A75, 7 pp. . 553 . 10.1051\/0004-6361\/201220967 . 2013A&A...553A..75C ,
3D modelling of HCO+ and its isotopologues in the low-mass proto-star IRAS16293-2422 . Quénard D. et al. . Monthly Notices of the Royal Astronomical Society, Volume 477, Issue 4, p.5312-5326 . 477 . 10.1093\/mnras\/sty1004 . 2018MNRAS.477.5312Q ,
Herschel spectral surveys of star-forming regions. Overview of the 555-636 GHz range . Ceccarelli C. et al. . Astronomy and Astrophysics, Volume 521, id.L22, 8 pp. . 521 . 10.1051\/0004-6361\/201015081 . 2010A&A...521L..22C ,
Instrument HIFI_HifiPoint_dbs, PACS_PacsRangeSpec_point, HIFI_HifiFS_freq
Temporal Coverage 2010-03-02T01:41:04Z/2012-02-25T10:32:47Z
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 2012-08-25T09:42:11Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2012-08-25T09:42:11Z, KPGT_cceccare_1, SPG v14.2.0. https://doi.org/10.5270/esa-jhvlcfb