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FAST Search for Atomic Hydrogen in Planetary Nebulae

Published online by Cambridge University Press:  06 October 2025

Yong Zhang*
Affiliation:
School of Physics and Astronomy, Sun Yat-sen University, Guangdong Province, China
Xu-Jia Ouyang
Affiliation:
School of Physics and Astronomy, Sun Yat-sen University, Guangdong Province, China
Albert Zijlstra
Affiliation:
Department of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK
Chuan-Peng Zhang
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China
Jun-ichi Nakashima
Affiliation:
School of Physics and Astronomy, Sun Yat-sen University, Guangdong Province, China
Quentin A. Parker
Affiliation:
Faculty of Science, The University of Hong Kong, Hong Kong, China

Abstract

Due to the contamination from omnipresent interstellar 21 cm emission, atomic hydrogen (H <sc>i</sc>) associated with planetary nebulae (PNe) has been insufficiently investigated. In this proceeding we report a project of searching for H i surrounding PNe using the Five hundred-meter Aperture Spherical radio Telescope (FAST), which is the most sensitive single-dish telescope at L-band. The observations may offer new insights into the interaction processes between PNe and the interstellar medium.

Information

Type
Poster Paper
Copyright
© The Author(s), 2025. Published by Cambridge University Press on behalf of International Astronomical Union

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References

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