Pre-stellar and Proto-stellar Cores and Cold Dust

Other

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

This proposal is designed to address several different scientific topics, the unifying theme of which is the search for and observation of nearby, very cold, dusty sources. We plan an imaging survey of pre-stellar cores to search for lower luminosity and/or younger sources than have been found in the IRAS and ISO data. Recent comparisons of pre-stellar and proto-stellar cores have indicated that they have fundamentally different structures: pre-stellar cores have not yet developed steep density gradients near their centers. These results were inferred from sub-millimeter observations of flux gradients in pre- and proto-stellar cores. MIPS has the capability for not only measuring flux gradients, but also temperature gradients and thus measuring much more directly the density gradients of the young cores to see whether this conclusion holds up. We plan an SED survey of some proto-stellar and pre-stellar cores to measure temperature and density gradients. Finally, MIPS is ideally suited to mapping far-infrared color temperatures, which we propose to do in a small number of clouds that have been well studied in the near-infrared and at other wavelengths. These data can be used to study the grain properties in the clouds.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Pre-stellar and Proto-stellar Cores and Cold Dust 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 Pre-stellar and Proto-stellar Cores and Cold Dust, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Pre-stellar and Proto-stellar Cores and Cold Dust will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1823351

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.