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researcher

V. Ramachandran

48 papers hereh-index 11506 citations56 works total

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

author position
  • sole author2
  • first author7
  • middle author34
  • last author1

Across the 44 of 48 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR37
  • astro-ph.GA8
  • astro-ph.HE2
  • physics.gen-ph1
same name
  • V. Ramachandran — 19 papers, h 50
  • V. Ramachandran — 15 papers, h 2
  • V. Ramachandran — 1 paper, h 7
  • V. Ramachandran — 1 paper, h 7
  • V. Ramachandran — 1 paper, h 5
  • V. Ramachandran — 1 paper, h 25

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
20172026
most citedThe Galactic WC and WO stars: The impact of revised distances from Gaia DR2 and their role as massive black hole progenitors

127 citations · 1.1k across the 46 of their papers we have counts for

collaborators
Showing 2026Show all

3 papers · 1 filter

astro-ph.SR2026

Distinct Population of Wolf-Rayet Stars in the Low-Metallicity Galaxy NGC 6822. Quantitative analysis of optical and UV spectra of the complete sample

R. Trigg, L. M. Oskinova, W. -R. Hamann +9

Context: Wolf-Rayet (WR) stars are particularly rare in low-metallicity galaxies and remain poorly understood. Detailed studies of the presumably complete population of WR stars in…

astro-ph.SR2026

Potsdam Wolf-Rayet stellar atmosphere grids of OB-type stars: I. Spectroscopic temperature diagnostics across metallicity

D. Pauli, H. Todt, W. -R. Hamann +5

Massive hot stars are among the major ionizing sources in the Universe. The ionizing flux of a star strongly depends on its temperature, which is best measured spectroscopically us…

physics.gen-ph2026

Multiplicity of Massive Stars at Low Metallicity: Early Results from the BLOeM Campaign

T. Shenar, J. Bodensteiner, M. Abdul-Masih +73

Massive stars at low metallicity (Z) play a central role in shaping the high-redshift Universe, yet their multiplicity remains poorly constrained. The Binarity at Low Metallicity (…

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