A dataset provided by the European Space Agency

Name: A STUDY OF M STARS WITH UNUSUAL MASS-LOSS RATES
Published: 1999-04-16T00:00:00Z

Name	PAW_2
Title	A STUDY OF M STARS WITH UNUSUAL MASS-LOSS RATES
URL	http://nida.esac.esa.int/nida-sl-tap/data?RETRIEVAL_TYPE=OBSERVATION&PRODUCT_LEVEL=ALL&obsno=125015180
DOI	https://doi.org/10.5270/esa-2uqmoye
Author	WHITELOCK, PATRICIA A
Description	we propose obtaining images of ten m stars with unusually high mass-loss rates. the objective is to examine their mass-loss histories and investigate the suggestion that they have recently undergone a helium shell flash.
Instrument	PHT03 , PHT04
Temporal Coverage	1996-03-20T10:21:57Z/1998-01-03T23:03:54Z
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, WHITELOCK et al., 1999, 'A STUDY OF M STARS WITH UNUSUAL MASS-LOSS RATES', 1.0, European Space Agency, https://doi.org/10.5270/esa-2uqmoye