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High-Speed Outflows and Dusty Disks during the AGB to PN Transition: The PANORAMA survey

Published online by Cambridge University Press:  06 October 2025

Raghvendra Sahai
Affiliation:
Jet Propulsion Laboratory, Pasadena, CA, USA
Javier Alcolea
Affiliation:
Observatorio Astronómico Nacional (IGN/CNIG), MITMA, Spain
Bruce Balick
Affiliation:
Dept. of Astronomy, University of Washington, Seattle, WA 98195-1580, USA
Eric G. Blackman
Affiliation:
Dept. of Physics & Astronomy, U. Rochester Rochester, NY, 14621, USA
Valentin Bujarrabal
Affiliation:
Observatorio Astronómico Nacional (IGN/CNIG), MITMA, Spain
Arancha Castro-Carrizo
Affiliation:
Institut de Radioastronomie Millimétrique, 300 rue de la Piscine, 38406 Saint-Martin-d’Heres, France
Orsola De Marco
Affiliation:
School of Mathematical and Physical Sciences, Macquarie University, Sydney, New South Wales, Australia
Joel H. Kastner
Affiliation:
Rochester Institute of Technology, Rochester, NY 14623 USA
Hyosun Kim
Affiliation:
Korea Astronomy and Space Science Institute, 776, Daedeokdae-ro, Yuseong-gu, Daejeon 34055, Republic of Korea
Eric Lagadec
Affiliation:
Université Côte d’Azur, CNRS, Boulevard de l’observatoire, CEDEX 4, 06304 Nice, France
Chin-Fei Lee
Affiliation:
Academia Sinica Institute of Astronomy and Astrophysics, No. 1, Sec. 4, Roosevelt Road, Taipei 106, Taiwan
Laurence Sabin
Affiliation:
Instituto de Astronomía, Universidad Nacional Autónoma de México, Apdo. Postal 877, C.P. 22860, Ensenada, B.C., México
M. Santander-García
Affiliation:
Observatorio Astronómico Nacional (IGN/CNIG), MITMA, Spain
Carmen Sánchez Contreras
Affiliation:
Centro de Astrobiología (CAB), CSIC-INTA. Postal address: ESAC, Camino Bajo del Castillo s/n, E-28692, Villanueva de la Cañada, Madrid, Spain
Daniel Tafoya
Affiliation:
Chalmers University of Technology, Onsala Space Observatory, Onsala, Sweden
Toshiya Ueta
Affiliation:
University of Denver, USA
Wouter Vlemmings
Affiliation:
Chalmers University of Technology, Onsala Space Observatory, Onsala, Sweden
Albert Zijlstra
Affiliation:
Jodrell Bank Centre for Astrophysics, Dept. of Physics and Astronomy, University of Manchester, Manchester, UK
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Abstract

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As AGB stars evolve to planetary nebulae (PNe), the geometry of the ejected mass transforms from nearly spherical to extremely aspherical. The mechanisms governing this transformation are plausibly linked to binarity and the associated production of disks and jets during the transitional (post-AGB) evolutionary stage. We are carrying out an ALMA survey of a representative sample of bipolar/multipolar post-AGB objects to obtain high angular-resolution (0″.11) observations of the CO(3–2) and 6–5 emission and study the collimated outflows and central disks. We present highlights from our ongoing survey – e.g., the presence of bipolar or multipolar high-velocity outflows, dense toroidal waists, and in one case, a circular ring around the central bipolar nebula. We will use radiative transfer modeling to derive accurate outflow momenta, masses, and mass-loss rates for our sample, thereby constraining different classes of binary PN-shaping models.

Information

Type
Contributed Paper
Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution and reproduction, provided the original article is properly cited.
Copyright
© The Author(s), 2025. Published by Cambridge University Press on behalf of International Astronomical Union

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