activity
20232026
collaborators

5 papers

astro-ph.GA2026

Individual Star Sampling in Star Formation Simulations: A Semi-Deterministic Model

Yunwei Deng, Hui Li, Zhiqiang Yan +2

In modern simulations that include star formation, it is common to use a universal and invariant initial mass function (IMF) to represent star populations or sample individual star…

astro-ph.GA2026

Limited imprint of high-mass IMF variations on sodium abundances in main-sequence galaxies

Ziyi Guo, Donatella Romano, Zhiqiang Yan +10

Growing evidence suggests that the stellar initial mass function (IMF) varies systematically across galaxies, deviating from the canonical Milky Way form. Such variations would mod…

astro-ph.GA2024

The Variation of the Galaxy-Wide IMF for Low-Mass Stars: Modeling and Observational Insights

Zhiqiang Yan, Jiadong Li, Pavel Kroupa +3

The Stellar Initial Mass Function (IMF) characterizes the mass distribution of newly formed stars in various cosmic environments, serving as a fundamental assumption in astrophysic…

astro-ph.GA2024

First detection of CO isotopologues in a high-redshift main-sequence galaxy: evidence of a top-heavy stellar initial mass function

Ziyi Guo, Zhi-Yu Zhang, Zhiqiang Yan +5

Recent observations and theories have presented a strong challenge to the universality of the stellar initial mass function (IMF) in extreme environments. A notable example has bee…

astro-ph.GA2023

The first ground-based detection of the 752 GHz water line in local ultra-luminous infrared galaxies using APEX-SEPIA

Daysi Quinatoa, Chentao Yang, Edo Ibar +10

We report the first ground-based detection of the water line p-H2O (211-202) at 752.033 GHz in three z < 0.08 ultra-luminous infrared galaxies (ULIRGs): IRAS 06035-7102, IRAS 17207…