scientific abstract this proposal sets out a plan for observations of the driving sources for herbig-haro (hh) flows, using both isophot-p and isophot-c to obtain maximum wavelength coverage. with the help of sub-mm observations, vital information on the evolution of disks around low-mass objects and their role in the mass loss phenomena can be derived. observation summary it is intended to perform broad band photometry on the energy sources with a variety of filters, but ensuring that there is always enough sky to allow background subtraction. in order to achieve 5% photometry, the minimum integration time per filter should be 32sec. this has, therefore, been selected as the standard integration time. with the pht-c detector a one-dimensional scans will be made at 200um, adding new science, possibly never again achievable. pht-p aot - pht03 peak-up required rectangular chopping - 60 throw filter aperture integration on source 10 23 32 12.8 23 32 16 23 32 20 23 32 25 23 32 pht-c aot - pht32 1x4 scan filter integration c200 14s per raster position (2s per chop step)
Instrument
PHT03 , PHT32
Temporal Coverage
1996-03-11T03:16:50Z/1996-03-24T09:29:33Z
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.
