Distance mapping technique and the 3-D structure of BD +30°3639
Abstract
We present a new kinematic analysis technique called distance mapping. It uses the observed proper motion vectors and the 3-D velocity field to determine the distance for each vector. From this information we generate maps that can be use as a constraint to morpho-kinematic modeling with SHAPE. It is applied to BD +30°3639, using the internal proper motion measurements by Li et al. (2002). We determine its distance at 1.40 kpc +/- 0.15 kpc.
- Publication:
-
Planetary Nebulae: An Eye to the Future
- Pub Date:
- August 2012
- DOI:
- 10.1017/S1743921312011143
- Bibcode:
- 2012IAUS..283..304A
- Keywords:
-
- ISM: jets and outflows;
- ISM: kinematics and dynamics;
- methods: numerical;
- planetary nebula: individual (BD +30°3639)