Spatially resolved 3 μm spectroscopy of IRAS 22272+5435

Details Spatially resolved 3 μm spectroscopy of IRAS 22272+5435 Spatially resolved 3 μm spectroscopy of IRAS 22272+5435

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003assl..283..243g&link_type=abstract

In: Mass-losing pulsating stars and their circumstellar matter. Workshop, May 13-16, 2002, Sendai, Japan, edited by Y. Nakada, M

Astronomy and Astrophysics

Astrophysics

Circumstellar Matter, Hydrocarbon Dust, Iras 22272+5435

Scientific paper

We present spatially resolved 3 μm spectroscopy of hydrocarbon dust in a proto-planetary nebula IRAS 22272+5435. The spectroscopy with adaptive optics system at the 8.2 m Subaru Telescope revealed intriguing spatial distribution of hydrocarbon molecules and dust. The intensity of aromatic hydrocarbon feature at 3.3 μm relative to the aliphatic-feature at 3.4 μm increases with the distance from the central star at 0".35-0".82 (560-1300 AU). The spectral variation is well reproduced by a sequence of spectra of a laboratory analog of hydrocarbon dust subjected to thermal annealing. It indicates that a similar thermal process takes place at the formation of hydrocarbon dust in IRAS 22272+5435.

Affiliated with

Also associated with

No associations

Rating

Spatially resolved 3 μm spectroscopy of IRAS 22272+5435 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 Spatially resolved 3 μm spectroscopy of IRAS 22272+5435, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spatially resolved 3 μm spectroscopy of IRAS 22272+5435 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-920649