Properties of Planetary Nebulae: NGC2022

Details Properties of Planetary Nebulae: NGC2022 Properties of Planetary Nebulae: NGC2022

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...20915608m&link_type=abstract

2007 AAS/AAPT Joint Meeting, American Astronomical Society Meeting 209, #156.08; Bulletin of the American Astronomical Society,

Other

2

Scientific paper

We present, for the planetary nebula NGC 2022, emission line flux mapping extracted from long-slit spectra taken with the 2.56 m Nordic Optical Telescope. Two-dimensional emission-line images for the entire nebula are created using data from only half of the nebula (which is symmetric), and are used to derive fluxes for 19 lines. We also create the Halpha/Hbeta extinction map, the [SII] and [Ar IV] line ratio density maps, and the [OIII] temperature map of the nebula. The total Hbeta flux is compared with values obtained by other authors. With these results we are now ready to begin modelling the nebula with a 3-D photoionization code, which will allow us to determine the 3-D structure, central star properties, and the distance to NGC 2022.

Affiliated with

Also associated with

No associations

Rating

Properties of Planetary Nebulae: NGC2022 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 Properties of Planetary Nebulae: NGC2022, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Properties of Planetary Nebulae: NGC2022 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1162188