activity
20022021
most citedDust Masses, PAH Abundances, and Starlight Intensities in the SINGS Galaxy Sample

1.1k citations · 1.8k across the 35 of their papers we have counts for

collaborators
Showing 2019Show all

7 papers · 1 filter

astro-ph.GA201915 cited

Fragmentation and isomerization of polycyclic aromatic hydrocarbons in the interstellar medium: coronene as a case study

Tao Chen, Yi Luo, Aigen Li

Aims. Due to the limitations of current computational technology, the fragmentation and isomerization products of vibrationally-excited polycyclic aromatic hydrocarbon (PAH) molecu…

astro-ph.IM201912 cited

The infrared bands of polycyclic aromatic hydrocarbons in the 1.6-1.7 μm wavelength region

Tao Chen, Yi Luo, Aigen Li

Context. The 3.3 m aromatic C-H stretching band of polycyclic aromatic hydrocarbon (PAH) molecules seen in a wide variety of astrophysical regions is often accompanied by a seri…

astro-ph.GA20199 cited

Probing the Missing Link between the Diffuse Interstellar Bands and the Total-to-Selective Extinction Ratio I. Extinction versus Reddening

Kaijun Li, Aigen Li, F. Y. Xiang

The carriers of the still (mostly) unidentified diffuse interstellar bands (DIBs) have been a long-standing mystery ever since their first discovery exactly 100 years ago. In recen…

astro-ph.GA201917 cited

How Much Graphene in Space?

Qi Li, Aigen Li, B. W. Jiang

The possible presence of graphene in the interstellar medium (ISM) is examined by comparing the interstellar extinction curve with the ultraviolet absorption of graphene calculated…

astro-ph.IM2019

Synthesizing carbon nanotubes in space

Tao Chen, Aigen Li

Context. As the 4th most abundant element in the universe, carbon (C) is widespread in the interstellar medium (ISM) in various allotropic forms (e.g., fullerenes have been identif…

astro-ph.HE2019

Two Numerical Methods for the 3D Anisotropic Propagation of Galactic Cosmic Rays

Wei Liu, Su-jie Lin, Hong-bo Hu +2

Conventional cosmic-ray propagation models usually assume an isotropic diffusion coefficient to account for the random deflection of cosmic rays by the turbulent interstellar magne…