pith. machine review for the scientific record. sign in

arxiv: 1809.06710 · v1 · submitted 2018-09-15 · 🌌 astro-ph.SR

Recognition: unknown

Morpho-Kinematics of the Circumstellar Environments around Post-AGB Stars

Authors on Pith no claims yet
classification 🌌 astro-ph.SR
keywords circumstellarenvironmentsmorpho-kinematicsrepresentingshellsourcealmaaround
0
0 comments X
read the original abstract

We observed two proto-planetary nebulae, HD 56126 representing a source with an elliptical circumstellar shell and IRAS 16594-4656 representing a source with a bipolar circumstellar shell, with ALMA in the 12CO and 13CO J=3-2 lines and neighboring continuum to see how the morpho-kinematics of CO gas and dust emission properties in their circumstellar environments differ.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.