The polarization of the infrared cluster in Orion - The spatial distribution of the 3.8 micron polarization

Other

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

98

Infrared Stars, Interstellar Matter, Optical Polarization, Orion Nebula, Polarization Characteristics, Spatial Distribution, Anisotropic Media, Astronomical Maps, Astronomical Spectroscopy, Cosmic Dust, Luminosity, Polarimetry, Polarized Radiation, Star Clusters

Scientific paper

A polarimetric map at L-prime (3.8 microns) has been prepared of a 40 arcsec region centered on the infrared cluster in Orion. The percentage of polarization exceeds 30 percent at many positions in the source. This fact, along with the systematic alignment of the polarization position angles, demonstrates that scattering is the principal polarization mechanism prevailing over most of the region. The Becklin-Neugebauer source and IRc2 are identified as the main sources responsible for illuminating the scattering grains. In addition, it is shown that the spatial distribution of dust in the immediate vicinity of IRc2 may be highly anisotropic. The results support the point of view that IRc2 is a highly luminous object, whereas others of the compact infrared sources may simply be isolated, nonluminous fragments of the cloud.

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

The polarization of the infrared cluster in Orion - The spatial distribution of the 3.8 micron polarization 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 The polarization of the infrared cluster in Orion - The spatial distribution of the 3.8 micron polarization, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The polarization of the infrared cluster in Orion - The spatial distribution of the 3.8 micron polarization will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1305880

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