A dataset provided by the European Space Agency

Name HII_SILI
Title SILICATE EMISSION FEATURES TOWARDS UCHII REGIONS
URL

http://nida.esac.esa.int/nida-sl-tap/data?RETRIEVAL_TYPE=OBSERVATION&PRODUCT_LEVEL=ALL&obsno=751012040

DOI https://doi.org/10.5270/esa-48en2ae
Author ROELFSEMA, PETER R
Description we propose an investigation of the properties of apparent silicate emission features in the ir spectra of ultra compact hii regions. with sws observations for the first time indications of such features towards hii region were seen. the relation of this material to the hii region is not at all clear. the proposed observations aim to significantly improve the signal to noise for these features, allowing a more detailed study of their properties and relation with the hii regions.
Instrument SWS06
Temporal Coverage 1997-11-30T01:03:46Z/1997-12-06T03:05:07Z
Version 1.0
Mission Description The Infrared Space Observatory (ISO) was the worlds first true orbiting infrared observatory. Equipped with four highly-sophisticated and versatile scientific instruments, it was launched by Ariane in November 1995 and provided astronomers world-wide with a facility of unprecedented sensitivity and capabilities for a detailed exploration of the Universe at infrared wavelengths.
Creator Contact https://support.cosmos.esa.int/iso/
Date Published 1999-04-08T00:00:00Z
Keywords ISO, infrared, SWS, LWS, ISOCAM, ISOPHOT
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, ROELFSEMA et al., 1999, 'SILICATE EMISSION FEATURES TOWARDS UCHII REGIONS', 1.0, European Space Agency, https://doi.org/10.5270/esa-48en2ae