PHT32 scans across the Dark Cloud L1166(CB236)

Details PHT32 scans across the Dark Cloud L1166(CB236) PHT32 scans across the Dark Cloud L1166(CB236)

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.482...87r&link_type=abstract

ISOPHOT: Proceedings of the Workshoip on P32 Oversampled Mapping, held in Madrid, Spain and Pasadena, CA, USA in February and Ma

Computer Science

Stars: Formation, Ism: Dust

Scientific paper

The results from the analysis of P32 scans at 100 m and 200 m across the dark cloud L1166(CB236) are presented and compared to previously analysed images from P22 raster maps of the region at the same wavelengths. It is found that the transient-corrected integrated flux densities (using P32TOOLS toolkit) of the cloud at the two wavelengths agree with those derived from the P22 maps within the errors. The dust tem- peratures derived from the two different observing modes both agree giving a temperature of 11.5K for an emissivity index (assuming ∝λ-β), β=2. Thus the P32 scans confirm that the dust is very cold indicating that the cloud is in a quiescent state and, assuming a distance of 300pc to the cloud, the estimated mass from the thermal dust emission is ~1.2 M_sun, in excellent agreement with submillimetre measurements.

Affiliated with

Also associated with

No associations

Rating

PHT32 scans across the Dark Cloud L1166(CB236) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with PHT32 scans across the Dark Cloud L1166(CB236), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and PHT32 scans across the Dark Cloud L1166(CB236) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-963365