A dataset provided by the European Space Agency

Name: Mass-losing AGB stars in the Small Magellanic Cloud
Published: 1999-04-16T00:00:00Z

Name	SMC_AGB
Title	Mass-losing AGB stars in the Small Magellanic Cloud
URL	http://nida.esac.esa.int/nida-sl-tap/data?RETRIEVAL_TYPE=OBSERVATION&PRODUCT_LEVEL=ALL&obsno=750003310
DOI	https://doi.org/10.5270/esa-3ereycr
Author	BLOMMAERT, JORIS A
Description	No abstract found for current proposal (This is a scientific proposal for an ESA mission. For specific information please contact ESDC Helpdesk - https://support.cosmos.esa.int/esdc)
Instrument	CAM01 , CAM04 , PHT03 , PHT22
Temporal Coverage	1996-09-09T23:51:32Z/1998-04-09T15:02:55Z
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	1999-04-16T00:00:00Z
Keywords	ISO, infrared, SWS, LWS, ISOCAM, ISOPHOT
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, BLOMMAERT et al., 1999, 'Mass-losing AGB stars in the Small Magellanic Cloud', 1.0, European Space Agency, https://doi.org/10.5270/esa-3ereycr