activity
19962026
most citedLSST Science Book, Version 2.0

924 citations · 6.6k across the 158 of their papers we have counts for

collaborators

158 papers

astro-ph.SR2026★ 1 cited

Current Unsolved Problems in Planetary Nebulae Research

Sun Kwok, Bruce Balick, You-Hua Chu +5

While there has been significant progress in our understanding of the origin and evolu-tion of planetary nebulae in the last 50 years, there remain several unsolved problems. These…

astro-ph.SR2023★ 1 cited

The porous envelope and circumstellar wind matter of the closest carbon star, CW Leonis

Hyosun Kim, Ho-Gyu Lee, Youichi Ohyama +5

Recent abrupt changes of CW Leonis may indicate that we are witnessing the moment that the central carbon star is evolving off the Asymptotic Giant Branch (AGB) and entering into t…

astro-ph.HE2023

Chandra Observation of NGC 1559: Eight Ultraluminous X-ray Sources Including a Compact Binary Candidate

Chen-Hsun Ma, Kwan-Lok Li, You-Hua Chu +1

Despite the 30-year history of ultra-luminous X-ray sources (ULXs) studies, issues like the majority of their physical natures (i.e., neutron stars, stellar-mass black holes, or in…

astro-ph.SR2023★ 7 cited

XMM-Newton Detection of X-ray Emission from the Metal-Polluted White Dwarf G 29-38

S. Estrada-Dorado, M. A. Guerrero, J. A. Toalá +3

A recent analysis of Chandra X-ray data of the metal-polluted white dwarf (WD) G29-38 has revealed X-ray emission that can be attributed to the accretion of debris from a planetary…

astro-ph.SR2023

The messy death of a multiple star system and the resulting planetary nebula as observed by JWST

Orsola De Marco, Muhammad Akashi, Stavros Akras +66

Planetary nebulae (PNe), the ejected envelopes of red giant stars, provide us with a history of the last, mass-losing phases of 90 percent of stars initially more massive than the…

astro-ph.GA2022★ 11 cited

Critical Metallicity of Cool Supergiant Formation. I. Effects on Stellar Mass Loss and Feedback

Po-Sheng Ou, Ke-Jung Chen, You-Hua Chu +1

This paper systematically studies the relation between metallicity and mass loss of massive stars. We perform one-dimensional stellar evolution simulations and build a grid of $\si…