activity
20232025
collaborators

5 papers

astro-ph.GA2025

A 3mm molecular line survey toward IRC+10216

Yi-Na Ao, Yong Zhang, Jian-Jie Qiu +2

IRC+10216 is the brightest infrared source in the northern sky, known for its rich chemical composition. It is often used as a standard reference for studying the circumstellar env…

astro-ph.GA2025

A molecule-rich torus-like structure in the 21 m source IRAS 23304+6147

Hao-Min Sun, Yong Zhang, Xu-Jia Ouyang +4

A long-standing enigma in observational astronomy is the identification of the so-called 21 m feature in a subset of envelopes of post-asymptotic giant branch (post-AGB) stars.…

astro-ph.GA2025

Considerations on the Origin of IRAS 19312+1950 Based on Long-Term Maser Observations

Huan-Xue Feng, Jun-ichi Nakashima, D. Engels +5

IRAS source 19312+1950 (hereafter I19312) is an infrared point source with maser emissions of SiO, HO, and OH molecules. Although initial observations suggested that I19312 mig…

astro-ph.SR2024

A 3 mm line survey towards the circumstellar envelope of the carbon-rich AGB star IRC+10216 (CW Leo)

Juan Tuo, Xiaohu Li, Jixian Sun +14

We present an unbiased 3 mm spectral line survey (between 84.5 and 115.8 GHz), conducted by the Purple Mountain Observatory 13.7 meter radio telescope, together with updated mo…

astro-ph.SR2023

Systematic Search for Water Fountain Candidates using the Databases of Circumstellar Maser Sources

Haichen Fan, Jun-ichi Nakashima, D. Engels +6

Water fountains (WFs) are thought to be objects in the morphological evolution of the circumstellar envelopes of low- and intermediate-mass evolved stars, transitioning from spheri…