A dataset provided by the European Space Agency

Name PROP_51
Title OBSERVATION OF NH3 IN SOME HOT MOLECULAR CORES AMMONIA IN HOT CORES
URL

http://nida.esac.esa.int/nida-sl-tap/data?RETRIEVAL_TYPE=OBSERVATION&PRODUCT_LEVEL=ALL&obsno=703002100

DOI https://doi.org/10.5270/esa-0icndqj
Author WALMSLEY, C M
Description ammonia observations at radio wavelengths have proved to be a useful probe of the physical parameters of dense molecular cores. we wish to test the models of the hot cores found in regions of massive star formation which are thought to be the birthplaces of o stars. we want to do this using the rotational transitions of ammonia which can be observed by the lws. we expect to observe absorption lines in many of our sources which will allow us to probe a different regime than that available to radio observers.
Instrument LWS01 , LWS03
Temporal Coverage 1997-05-24T05:25:00Z/1997-10-20T17:43:10Z
Version 1.0
Mission Description The Infrared Space Observatory (ISO) was the world's 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 1999-01-20T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, WALMSLEY, C M, 1999, PROP_51, 1.0, European Space Agency, https://doi.org/10.5270/esa-0icndqj