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 2017Show all

6 papers · 1 filter

astro-ph.GA2017

Cosmic Dust IX

Hiroshi Kimura, Ludmilla Kolokolova, Aigen Li +3

This is an editorial to the special issue on Cosmic Dust IX.

astro-ph.GA201723 cited

On Graphene in the Interstellar Medium

X. H. Chen, Aigen Li, Ke Zhang

The possible detection of C_{24}, a planar graphene, recently reported in several planetary nebulae by Garciaa-Hernandez et al. (2011, 2012) inspires us to explore whether and how…

astro-ph.GA201724 cited

Interstellar Silicon Depletion and the Ultraviolet Extinction

Ajay Mishra, Aigen Li

Spinning small silicate grains were recently invoked to account for the Galactic foreground anomalous microwave emission. These grains, if present, will absorb starlight in the far…

astro-ph.GA2017114 cited

The gas-to-extinction ratio and the gas distribution in the Galaxy

Hui Zhu, Wenwu Tian, Aigen Li +1

We investigate the relation between the optical extinction () and the hydrogen column density () determined from X-ray observations of a large sample of Galactic sightlin…

astro-ph.GA201714 cited

Detection of Polarized Infrared Emission by Polycyclic Aromatic Hydrocarbons in the MWC 1080 Nebula

Han Zhang, Charles M. Telesco, Thiem Hoang +5

Polycyclic aromatic hydrocarbons (PAHs) are ubiquitous in astrophysical environments, as revealed by their pronounced emission features at 3.3, 6.2, 7.7, 8.6, 11.3, and 12.7 m c…

astro-ph.GA201726 cited

Polycyclic Aromatic Hydrocarbons with Aliphatic Sidegroups: Intensity Scaling for the C-H Stretching Modes and Astrophysical Implications

Xuejuan Yang, Aigen Li, R. Glaser +1

The so-called unidentified infrared emission (UIE) features at 3.3, 6.2, 7.7, 8.6, and 11.3 m ubiquitously seen in a wide variety of astrophysical regions are generally attribut…