scientific abstract the prime scientific goal is to obtain precise, well spectrally sampled absolute photometry in the 2.5 - 200 microns wavelength range of a complete sample of a compact dense condensations of cold dust and gas, selected by sensitive, high angular resolution surveys of cloud cores at mm/sub mm wavelengths. the high precision fir/mir spectra, supplemented by mir/nir diffraction limited imaging, will differentiate between various evolutionary stages, allowing true isothermal protostars, disk and cocoon stars to be distinguished from one another. the relative detection rate of these phenomena will reflect the true incidence of these objects within each of the cloud cores surveyed in the submm, and will therby allow statements to be made about the duration of the evolutionary stages of star formation. observation summary for investigation of nearby protostar candidates and their parent clouds: p25 rasters of subfields (3x3 up to 7x7 depending on cloud size) at 200, 100, 60 micron with tint = 5s. raster step interval = array repeat length (180, 138 arcsec for c200, c100). to be performed concatenated. for each individual protostar candidate within cloud, perform concatenated: p05 1x11,1x10 rasters at 25 micron, using 10 arcsec aperture and minimal raster step of 10 arcsec. the sum of these will provide 5 sampling over a 100 scanlength. to provide information about the background outside the cloud an additional p05 1x7 raster with 50 raster step is proposed. all p05 rasters use tint=5s. p32 at 200, 160, 120 micron (4x2)raster, o/s 2, tint = 10s per s/c raster point p32 at 100, 70, 60 micron (4x2)raster, o/s 2/3, tint = 10s per s/c raster point p40 in a 5x1 raster tint = 32s. (raster interval chosen to provide 1 point on protostar candidate, 2 points on parent cloud, 2 points on ba...ckground) for investigation of distant star forming clouds we propose the following: p25 rasters of subfields (3x3) 200, 100, 60 micron with tint = 5s. raster step interval = array repeat length (180, 138 arcsec for c200, c100). centered at the cloud core, perform concatenated: p05 1x5 raster at 25 micron, using tint=5s and 23 arcsec aperture (raster interval chosen to provide 1 point on cloud core, 2 points on cloud, 2 points on background) p40 in an identical 5x1 raster tint = 32s. p32 at 200, 160, 120 micron (4x2)raster, o/s 2, tint = 10s per s/c raster point p32 at 100, 60 micron (4x2)raster, o/s 2/3, tint = 10s per s/c raster point
Instrument
PHT03 , PHT32 , PHT40
Temporal Coverage
1996-09-06T22:20:23Z/1998-02-27T18:30:08Z
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.
European Space Agency, 1999, Iso Observations Of The Earliest Evolutionary Stages Of Protostars Part 1 Of 3 , 1.0, European Space Agency, https://doi.org/10.5270/esa-b1qwg2u
