A dataset provided by the European Space Agency

Name OT2_hbeuther_4
Title Formation signatures and carbon budget of molecular clouds
URL

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342270620&instrument_name=HIFI&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342270621&instrument_name=HIFI&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342270624&instrument_name=HIFI&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342270625&instrument_name=HIFI&product_level=LEVEL0&compress=true

DOI https://doi.org/10.5270/esa-af0hgr7
Author beuther, h.
Description The interstellar medium (ISM) is mainly comprised of ionized, neutralatomic and molecular gas. One of the most important constituents ofthese phases is carbon in its ionized/neutral/molecular form (C^+, C^0and CO). However, a coherent analysis of the different phases atadequate resolution (Jeans length virgul0.2pc) is lacking. We thereforewant to re-evaluate the ISM carbon budget via observing primarily C^+at 1.9THz, C^0 (at 492GHz), and CO(2-1) with Herschel, APEX and theIRAM 30m at high spatial resolution (11.-13.) for several infrareddark clouds (IRDCs). This proposal is a follow-up of a guaranteedtime pilot study for the line of ionized carbon CII toward oneIRDC. In this open time project we like to extend the sample to atotal of five IRDCs in different environments. With the combined dataof the different carbon phases we can address: (a) How do the relativeabundances change with evolutionary stage? (b) Are the differentphases mainly excited by internal or external radiation sources? (c)How important are the phase changes for the carbon cooling budget ofthe ISM? (d) Can we identify cloud formation signatures (e.g.,turbulent flows)?
Publication
  • Carbon in different phases (CII, CI, and CO) in infrared dark clouds: Cloud formation signatures and carbon gas fractions | Beuther H. et al. | Astronomy & Astrophysics Volume 571 id.A53 15 pp. | 571 | 10.1051\\/0004-6361\\/201424757 | 2014A&A...571A..53B | http://adsabs.harvard.edu/abs/2014A%26A...571A..53B
Instrument HIFI_HifiMapping_load-raster
Temporal Coverage 2013-04-18T18:36:07Z/2013-04-19T09:59:04Z
Version SPG v14.1.0
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 2013-10-19T07:40:30Z
Keywords Herschel, HSC, submillimetre, far-infrared, HIFI, PACS, SPIRE
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, beuther et al., 2013, 'Formation signatures and carbon budget of molecular clouds', SPG v14.1.0, European Space Agency, https://doi.org/10.5270/esa-af0hgr7