Investigating Circumstellar Disk Geometry and Dust Properties with Coronagraphic Polarimetry

Physics – Optics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

1

Circumstellar Shells, Clouds, And Expanding Envelopes, Circumstellar Masers, Photometric, Polarimetric, And Spectroscopic Instrumentation, Interstellar Dust Grains, Diffuse Emission, Infrared Cirrus, Astrometric And Interferometric Instruments

Scientific paper

High angular resolution coronagraphy and imaging polarimetry have both proved to be valuable tools for studying the properties of circumstellar disks around young stars, but only recently has it become possible to combine these techniques together. Coronagraphic polarimetry observations, obtainable with ACS and NICMOS on the Hubble Space Telescope, and some adaptiveoptics-corrected telescopes on the ground, are now providing new constraints on light scattered on sub-arcsecond scales within disks. When combined with multiwavelength numerical radiative transfer models, these data can yield insight into both the overall disk geometry as well as the size distribution and other properties of their constituent dust grains. We present initial results from several recent HST programs studying disks around young stars, summarize ongoing modeling efforts, and discuss future prospects.

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

Investigating Circumstellar Disk Geometry and Dust Properties with Coronagraphic Polarimetry 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 Investigating Circumstellar Disk Geometry and Dust Properties with Coronagraphic Polarimetry, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Investigating Circumstellar Disk Geometry and Dust Properties with Coronagraphic Polarimetry will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1313545

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