A dataset provided by the European Space Agency

Name YSO_OUT
Title PHYSICAL PROPERTIES OF OUTFLOWS FROM YOUNG STELLAR OBJECTS PROBING THE CIRCUMSTELLAR ENVIRONMENT
URL

http://nida.esac.esa.int/nida-sl-tap/data?RETRIEVAL_TYPE=OBSERVATION&PRODUCT_LEVEL=ALL&obsno=296001020

DOI https://doi.org/10.5270/esa-9sm1hlq
Author HIRTH, GERHARD A
Description this research proposal aims at a better understanding of the physical properties of mass outflows from young stellar objects in different evolutionary stages. using iso.s lws we expect to gain new information concerning the nature of the driving source, the mass loss rate, the collimation, the excitation condition in the outflow region and the physical properties of the circumstellar mass distribution. furthermore, with the new data we hope to discriminate among conflicting models by constraining their parameter spaces. we request 9 hours for line scans at medium and high resolution (autumn launch). for spring launch 8.2 hours are foreseen.
Instrument LWS01 , LWS02 , LWS04
Temporal Coverage 1996-09-07T15:06:18Z/1996-11-14T18:03:10Z
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 1999-05-29T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, HIRTH, GERHARD A, 1999, YSO_OUT, 1.0, European Space Agency, https://doi.org/10.5270/esa-9sm1hlq