A dataset provided by the European Space Agency

Name: BARS AND TIDES IN GALAXIES ROLE OF LARGE-SCALE DYNAMICS ON STAR FORMATION
Published: 1999-04-08T00:00:00Z

Name	BAR_TIDA
Title	BARS AND TIDES IN GALAXIES ROLE OF LARGE-SCALE DYNAMICS ON STAR FORMATION
URL	http://nida.esac.esa.int/nida-sl-tap/data?RETRIEVAL_TYPE=OBSERVATION&PRODUCT_LEVEL=ALL&obsno=184020270
DOI	https://doi.org/10.5270/esa-gbroymi
Author	COMBES, F B
Description	the main aim is to study the effects of the presence of a nearby companion, and of a central bar (i.e. the effects of gravitational perturbations) on the gas properties and star-formation activity in spiral galaxies. this kind of statistical study has been carried out in the radio-continuum emission, in halpha and in co emission: the inter-comparison of these results with fir lines will allow a deeper understanding of large-scale physical processes leading to star formation.
Instrument	LWS02
Temporal Coverage	1996-04-27T05:22:25Z/1997-09-02T00:50:58Z
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	1999-04-08T00:00:00Z
Keywords	ISO, infrared, SWS, LWS, ISOCAM, ISOPHOT
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, COMBES et al., 1999, 'BARS AND TIDES IN GALAXIES ROLE OF LARGE-SCALE DYNAMICS ON STAR FORMATION', 1.0, European Space Agency, https://doi.org/10.5270/esa-gbroymi