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G. Harris

4 papers hereh-index 5231 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
  • G. Harris — 10 papers, h 28
  • G. Harris — 1 paper, h 0
  • G. Harris — 1 paper, h 11

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
20032006
most citedSpitzer spectroscopy of carbon stars in the Small Magellanic Cloud

82 citations · 88 across the 2 of their papers we have counts for

collaborators

4 papers

astro-ph2006★ 82 cited

Spitzer spectroscopy of carbon stars in the Small Magellanic Cloud

Eric Lagadec, Albert A. Zijlstra, G. C. Sloan +12

We present Spitzer Space telescope spectroscopic observations of 14 carbon-rich AGB stars in the Small Magellanic Cloud. SiC dust is seen in most of the carbon-rich stars but it is…

astro-ph2006★ 6 cited

Non-grey hydrogen burning evolution of sub-Solar mass Population III stars

G. J. Harris, A. E. Lynas-Gray, S. Miller +1

The primordial elements, H, He and Li are included in a low temperature equation of state and monochromatic opacity function. The equation of state and opacity function are incorpo…

astro-ph2004

The role of HeH+ in cool helium rich white dwarfs

G. J. Harris, A. E. Lynas-Gray, S. Miller +1

HeH+ is found to be the dominant positive ion over a wide range of temperatures and densities relevant to helium rich white dwarfs. The inclusion of HeH+ in ionization equili…

astro-ph2003

The effect of the electron donor H3+ on the pre-main and Main Sequence evolution of low mass zero metallicity stars

G. J. Harris, A. E. Lynas-Gray, S. Miller +1

H3+ has been shown (Lenzuni et al. 1991, ApJS, 76, 759) to be the dominant positive ion, in a zero metallicity gas at low temperature and intermediate to high density. It therefore…

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