A dataset provided by the European Space Agency

Name DDT_tphill01_2
Title H2O Strip Towards Sagittarius B2: Unveiling the Enhancement Properties of Water Abundance Towards the Galactic Center
URL

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342243698&instrument_name=HIFI&product_level=LEVEL0&compress=true

DOI 10.5270/esa-refajrl
Author phillips, t.
Description HerschelHIFI results suggest that hydrogen fluoride abundance is comparable to that of para-water over much of the interstellar medium, but not in the galactic center region where an enhancement of water abundance is observed. As part of the HEXOS GT KP, a strip scan of HF of a region of size 2" north and south towards the massive star-forming region of Sagittarius B2 (M) has been observed. We propose observations of a strip map of the para-H _2 O fundamental line towards the same region. The H _2 O strip would be extremely valuable to compare the spatial variations between HF and H _2 O and will allow us to study the nature of the water abundance enhancement towards the galactic center.
Publication
Instrument HIFI_HifiMapping_raster
Temporal Coverage 2012-04-04T02:16:49Z/2012-04-04T04:21:09Z
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 ┬Ám range, bridging the gap between earlier infrared space missions and groundbased facilities.
Creator Contact https://support.cosmos.esa.int/herschel/
Date Published 2012-10-04T02:16:49Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2012-10-04T02:16:49Z, DDT_tphill01_2, SPG v14.1.0. https://doi.org/10.5270/esa-refajrl