ngc 604 is the brightest star-formation complex in the nearby spiral m 33. it will be observed in the central programme with cam (filter imaging), phot, lws and sws. in order to help interpret the cam filter imaging and obtain more information on the properties of gas and dust in this complex object, we propose an observation with the cam cvf: it will map unambiguously the different unidentified infrared bands and several fine-structure lines, which are not well separated by the cam filters. we expect to see a wealth of details with the resolution of 6.
Instrument
CAM04
Temporal Coverage
1998-01-09T21:02:31Z/1998-01-09T23:16:51Z
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.
European Space Agency, VIALLEFOND et al., 1999, 'CAM-CVF OBSERVATIONS OF NGC 604 IN THE NEARBY GALAXY M 33', 1.0, European Space Agency, https://doi.org/10.5270/esa-d4ymayo
