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D. Allen

7 papers hereh-index 7228 citations15 works total

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

author position
  • first author5
  • last author2

Across the 7 of 7 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR4
  • astro-ph3
same name
  • D. Allen — 15 papers, h 8
  • D. Allen — 5 papers, h 5
  • D. Allen — 2 papers, h 6
  • D. Allen — 2 papers, h 1
  • D. Allen — 2 papers, h 1
  • D. Allen — 1 paper, h 8

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
20062018
most citedElemental abundances and classification of CEMP stars

94 citations · 294 across the 7 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

4 papers · 1 filter

astro-ph.SR2018★ 33 cited

Iron-peak elements Sc, V, Mn, Cu and Zn in Galactic bulge globular clusters

H. Ernandes, B. Barbuy, A. Alves-Brito +3

Globular clusters are tracers of the history of star formation and chemical enrichment in the early Galaxy. Their abundance pattern can help understanding their chemical enrichment…

astro-ph.SR2012★ 94 cited

Elemental abundances and classification of CEMP stars

Dinah M. Allen, Sean G. Ryan, Silvia Rossi +2

We present a detailed study of Carbon-Enhanced Metal-Poor (CEMP) stars, based on high-resolution spectroscopic observations of a sample of 18 stars. The stellar spectra for this sa…

astro-ph.SR2010★ 23 cited

Mn, Cu and Zn abundances in barium stars and their correlations with neutron capture elements

Dinah M. Allen, Gustavo F. Porto de Mello

We present abundances of Mn, Cu, Zn and various light and heavy elements for a sample of barium and normal giant stars, and present correlations between abundances contributed to d…

astro-ph.SR2009★ 7 cited

HD 11397 and HD 14282 - Two new barium stars?

L. Pompeia, D. M. Allen

We have performed a detailed abundance analysis of the content of s-process elements of two dwarf stars with suspected overabundace of those elements. Such stars belong to a specia…

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