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researcher

V. Hill

139 papers hereh-index 6514.6k citations343 works total

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

author position
  • first author6
  • middle author101
  • last author8

Across the 115 of 139 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA64
  • astro-ph32
  • astro-ph.SR28
  • astro-ph.IM12
  • astro-ph.CO3
same name
  • V. Hill — 23 papers, h 7
  • V. Hill — 20 papers, h 16
  • V. Hill — 13 papers, h 8
  • V. Hill — 10 papers, h 7
  • V. Hill — 5 papers, h 5
  • V. Hill — 2 papers, h 14

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
19992023
most citedFirst stars V - Abundance patterns from C to Zn and supernova yields in the early Galaxy

1.2k citations · 16.7k across the 138 of their papers we have counts for

collaborators
Showing 2003Show all

3 papers · 1 filter

astro-ph2003★ 1.2k cited

First stars V - Abundance patterns from C to Zn and supernova yields in the early Galaxy

R. Cayrel, E. Depagne, M. Spite +11

In the framework of an ESO Large Programme high quality spectra of 70 very metal-poor dwarfs and giants were obtained with the VLT-UVES combination. This paper reports the detailed…

astro-ph2003★ 115 cited

First stars IV.CS 29497-030: Evidence for operation of the s-process at very low metallicity

T. Sivarani, P. Bonifacio, P. Molaro +12

We present an abundance analysis of the very metal-poor, carbon-enhanced star CS 29497-030. Our results indicate that this unusually hot turnoff star (Teff = 6650K, log g = 3.5) ha…

astro-ph2003★ 549 cited

The Extremely Metal-Poor, Neutron-Capture-Rich Star CS 22892-052: A Comprehensive Abundance Analysis

C. Sneden, J. J. Cowan, J. E. Lawler +9

High-resolution spectra obtained with three ground-based facilities and the Hubble Space Telescope (HST) have been combined to produce a new abundance analysis of CS 22892-052, an…

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