English

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

Solar and Stellar Astrophysics 2018-09-19 v1

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.

Keywords

Cite

@article{arxiv.1809.06710,
  title  = {Morpho-Kinematics of the Circumstellar Environments around Post-AGB Stars},
  author = {Toshiya Ueta and Hideyuki Izumiura and Issei Yamamura and Masaaki Otsuka},
  journal= {arXiv preprint arXiv:1809.06710},
  year   = {2018}
}

Comments

2 pages, 2 figures; contribution to Proceedings of IAU Symp 343