A dataset provided by the European Space Agency

Name: EVOLUTION AND MASS LOSS OF AGB STARS IN THE SMALL MAGELLANIC CLOUD
Published: 1998-12-18T00:00:00Z

Name	S13_PHT
Title	EVOLUTION AND MASS LOSS OF AGB STARS IN THE SMALL MAGELLANIC CLOUD
URL	http://nida.esac.esa.int/nida-sl-tap/data?RETRIEVAL_TYPE=OBSERVATION&PRODUCT_LEVEL=ALL&obsno=750004010
DOI	https://doi.org/10.5270/esa-l7sh2nk
Author	BLOMMAERT, JORIS A
Description	in a study (based on near-infrared and iso data) of agb stars in the smc we discovered an unusual object with a very high mass loss rate (approx 10^(-4) msun/year) but only a modest to low luminosity (about 5300 lsun). to more accurately determine its luminosity and investigate the mass loss history of this star we propose 60 and 100 micron observations with pht.
Instrument	PHT22
Temporal Coverage	1997-12-04T15:07:09Z/1997-12-04T15:32:51Z
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	1998-12-18T00:00:00Z
Keywords	ISO, infrared, SWS, LWS, ISOCAM, ISOPHOT
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, BLOMMAERT et al., 1998, 'EVOLUTION AND MASS LOSS OF AGB STARS IN THE SMALL MAGELLANIC CLOUD', 1.0, European Space Agency, https://doi.org/10.5270/esa-l7sh2nk