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Aigen Li

31 papers hereh-index 202.9k citations29 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author18
  • last author5

Across the 23 of 31 papers where every author was matched, so the position is known.

fields
  • astro-ph18
  • astro-ph.GA8
  • astro-ph.CO4
  • astro-ph.SR1
same name
  • Aigen Li — 131 papers, h 35
  • Aigen Li — 14 papers, h 5
  • Aigen Li — 7 papers
  • Aigen Li — 4 papers, h 4
  • Aigen Li — 4 papers, h 1
  • Aigen Li — 2 papers, h 2

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20032026
most citedSINGS: The SIRTF Nearby Galaxies Survey

1.3k citations · 3.8k across the 31 of their papers we have counts for

collaborators
Showing 2008Show all

4 papers · 1 filter

astro-ph2008★ 112 cited

Dust Processing and Grain Growth in Protoplanetary Disks in the Taurus-Auriga Star-Forming Region

B. A. Sargent, W. J. Forrest, C. Tayrien +9

Mid-infrared spectra of 65 T Tauri stars (TTS) taken with the Infrared Spectrograph (IRS) on board the Spitzer Space Telescope are modeled using dust at two temperatures to probe t…

astro-ph2008★ 96 cited

Silica in Protoplanetary Disks

B. A. Sargent, W. J. Forrest, C. Tayrien +10

Mid-infrared spectra of a few T Tauri stars (TTS) taken with the Infrared Spectrograph (IRS) on board the Spitzer Space Telescope show prominent narrow emission features indicating…

astro-ph2008★ 47 cited

On Dust Extinction of Gamma-ray Burst Host Galaxies

Aigen Li, S. L. Liang, D. A. Kann +3

Although it is well recognized that gamma-ray burst (GRB) afterglows are obscured and reddened by dust in their host galaxies, the wavelength-dependence and quantity of dust extinc…

astro-ph2008★ 124 cited

The relations among 8, 24, and 160 micron dust emission within nearby spiral galaxies

G. J. Bendo, B. T. Draine, C. W. Engelbracht +9

We investigate the relations among the stellar continuum-subtracted 8 micron polycyclic aromatic hydrocarbon (PAH 8 micron) emission, 24 micron hot dust emission, and 160 micron co…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.