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K. Chan

4 papers hereh-index 6328 citations14 works total

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

author position
  • first author2
  • middle author1

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph4
same name
  • K. Chan — 164 papers, h 87
  • K. Chan — 37 papers, h 17
  • K. Chan — 27 papers, h 18
  • K. Chan — 18 papers
  • K. Chan — 17 papers, h 13
  • K. Chan — 14 papers, h 7

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
19982001
most citedGlobal Physical Conditions of the Interstellar Medium in Nearby Galaxies

94 citations · 94 across the 1 of their papers we have counts for

collaborators

4 papers

astro-ph2001★ 94 cited

Global Physical Conditions of the Interstellar Medium in Nearby Galaxies

T. Negishi, T. Onaka, K. -W. Chan +1

Far-infrared spectra (43-197um) of 34 nearby galaxies obtained by the Long Wavelength Spectrometer (LWS) aboard the Infrared Space Observatory (ISO) were analyzed to investigate th…

astro-ph2000

Unidentified Infrared Emission Bands in the Diffuse Interstellar Medium

Kin-Wing Chan, T. L. Roellig, T. Onaka +7

Using the Mid-Infrared Spectrometer on board the Infrared Telescope in Space and the low-resolution grating spectrometer (PHT-S) on board the Infrared Space Observatory, we obtaine…

astro-ph2000

A Broad 22 Microns Emission Feature in the Carina Nebula H II Region

K. -W. Chan, T. Onaka

We report the detection of a broad 22 microns emission feature in the Carina nebula H II region by the Infrared Space Observatory (ISO) Short Wavelength Spectrometer. The feature s…

astro-ph1998

The Nature of the Mid-Infrared Background Radiation in the Galactic Bulge from the IRTS Observations

K. W. Chan, T. L. Roellig, T. Onaka +2

Using the Mid-Infrared Spectrometer (MIRS) on board the Infrared Telescope in Space (IRTS) we obtained the 4.5 to 11.7 micron spectra of the stellar populations and diffuse interst…

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