High spatial resolution 10 micron imaging of IRC + 10216

Details High spatial resolution 10 micron imaging of IRC + 10216 High spatial resolution 10 micron imaging of IRC + 10216

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...333..300b&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 333, Oct. 1, 1988, p. 300-304.

Astronomy and Astrophysics

Astrophysics

18

Carbon Stars, Infrared Stars, Linear Arrays, Spatial Resolution, Brightness Distribution, Computerized Simulation, Cosmic Dust, Stellar Envelopes, Stellar Mass Ejection

Scientific paper

Precise high-resolution 10-micron images of the carbon star IRC + 10216 have been obtained with a scanned linear array. The low noise and high dynamic range of these images permit deconvolution of the telescope point-spread function, revealing the radial brightness distribution of the circumstellar dust shell: approximate reflection symmetry is found in west-east scans, with a distinct division into two components of diameter about 0.40 and 2.2 arcsec. It is shown that this morphology is consistent with published interferometric data that had cast doubt upon an earlier, idealized two-component model. The observed brightness distribution implies that the circumstellar dust density may deviate substantially from the 1/r squared radial dependence expected for spherically symmetric outflow with constant velocity and constant rate of mass loss.

Affiliated with

Also associated with

No associations

Rating

High spatial resolution 10 micron imaging of IRC + 10216 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 High spatial resolution 10 micron imaging of IRC + 10216, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High spatial resolution 10 micron imaging of IRC + 10216 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1598096