3-D Structure of the H2 Emission of CRL 2688

Details 3-D Structure of the H2 Emission of CRL 2688 3-D Structure of the H2 Emission of CRL 2688

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..804...96m&link_type=abstract

PLANETARY NEBULAE AS ASTRONOMICAL TOOLS: International Conference on Planetary Nebulae as Astronomical Tools. AIP Conference Pr

Astronomy and Astrophysics

Astronomy

H Ii Regions, Giant Stars, Nebulae, Stellar Structure, Hii Regions, Emission And Reflection Nebulae, Giant And Subgiant Stars, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages

Scientific paper

We present the spatial structure of the H2 emission of the post-AGB star CRL 2688 reconstructed from a series of images of high spatial resolution (~ 0.2'') allowing observations from different line of sights and, with an unprecedented clarity, the true structure of this nebula. CRL 2688 presents a helicoidal structure. This structure could be interpreted as resulting from a bipolar outflow in the north-south direction linked to the rotation of the nebula along its polar axis.

Affiliated with

Also associated with

No associations

Rating

3-D Structure of the H2 Emission of CRL 2688 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 3-D Structure of the H2 Emission of CRL 2688, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and 3-D Structure of the H2 Emission of CRL 2688 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1834839