Near-infrared Observations of the Proto-Planetary Nebula IRAS 07131-0147

Mathematics – Logic

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

We present J and K images obtained under photometric conditions with the Lick 3m telescope of the Proto-Planetary Nebula IRAS 07131-0147 (galactic coordinates l=217, b=+4.7). This highly polarized bipolar reflection nebula is believed to be in the poorly understood evolutionary transition from the Asymptotic Giant Branch to Planetary Nebula. We find IRAS 07131-0147 to exhibit point reflection symmetry - a morphological characteristic rarely found in bipolar nebulae. Utilizing numerical integrations of single grain scattering models we derive a nearly face-on inclination angle of i < 5 degrees. The (J-K) color indicates that the central star (type M5 III) is negligibly reddened consistent with the `mid-butterfly' classification of the nebula (where the central star is relatively unobscured). Using the mean K magnitude of M5 galactic bulge giants, we estimate an approximate distance of 6 +/- 2 kpc, making this one of the most distant Proto-Planetary Nebulae known.

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

Near-infrared Observations of the Proto-Planetary Nebula IRAS 07131-0147 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 Near-infrared Observations of the Proto-Planetary Nebula IRAS 07131-0147, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Near-infrared Observations of the Proto-Planetary Nebula IRAS 07131-0147 will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1255897

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