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Richard I. Anderson

2 papers hereh-index 230 citations2 works total

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

author position
  • middle author2

Across the 2 of 2 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA1
  • astro-ph.SR1
same name
  • Richard I. Anderson — 8 papers, h 4
  • Richard I. Anderson — 8 papers, h 3
  • Richard I. Anderson — 4 papers
  • Richard I. Anderson — 4 papers, h 0
  • Richard I. Anderson — 3 papers, h 2
  • Richard I. Anderson — 3 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

most citedThe magnetic strip(s) in the advanced phases of stellar evolution - Theoretical convective turnover timescale and Rossby number for low- and intermediate-mass stars up to the AGB at various metallicities

41 citations · 48 across the 2 of their papers we have counts for

collaborators

2 papers

astro-ph.GA2024★ 7 cited

On the dynamical evolution of Cepheid multiplicity in star clusters and its implications for B-star multiplicity at birth

František Dinnbier, Richard I. Anderson, Pavel Kroupa

Classical Cepheid variable stars provide a unique probe to binary evolution in intermediate-mass stars over the course of several tens to hundreds of Myr. We studied the binary and…

astro-ph.SR2017★ 41 cited

The magnetic strip(s) in the advanced phases of stellar evolution - Theoretical convective turnover timescale and Rossby number for low- and intermediate-mass stars up to the AGB at various metallicities

C. Charbonnel, T. Decressin, N. Lagarde +7

Recent spectropolarimetric observations of otherwise ordinary G, K, and M giants revealed localized magnetic strips in the HRD coincident with the regions where the first dredge-up…

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