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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 astro-ph.HEShow all

2 papers · 1 filter

astro-ph.HE2024★ 4 cited

Multi-wavelength spectroscopic analysis of the ULX Holmberg II X-1 and its nebula suggests the presence of a heavy black hole accreting from a B-type donor

S. Reyero Serantes, L. Oskinova, W. -R. Hamann +11

Ultra-luminous X-ray sources (ULXs) are high-mass X-ray binaries with an X-ray luminosity above 1039 erg s−1. These ULXs can be powered by black holes that are more massi…

astro-ph.HE2022★ 22 cited

Phase-resolved spectroscopic analysis of the eclipsing black hole X-ray binary M33 X-7: System properties, accretion, and evolution

V. Ramachandran, L. M. Oskinova, W. -R. Hamann +10

M33 X-7 is the only known eclipsing black hole high mass X-ray binary. The system is reported to contain a very massive O supergiant donor and a massive black hole in a short orbit…

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