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researcher

A. Sander

52 papers hereh-index 10379 citations55 works total

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

author position
  • first author2
  • middle author44
  • last author2

Across the 48 of 52 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR39
  • astro-ph.GA7
  • astro-ph.HE4
  • astro-ph.IM1
  • physics.gen-ph1
same name
  • A. Sander — 86 papers, h 55
  • A. Sander — 40 papers, h 30
  • A. Sander — 20 papers, h 2
  • A. Sander — 16 papers, h 4
  • A. Sander — 14 papers, h 16
  • A. Sander — 6 papers

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
20132026
most citedPoWR grids of non-LTE model atmospheres for OB-type stars of various metallicities

87 citations · 774 across the 49 of their papers we have counts for

collaborators
Showing 2022Show all

3 papers · 1 filter

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…

astro-ph.SR2022★ 36 cited

Stellar wind properties of the nearly complete sample of O stars in the low metallicity young star cluster NGC346 in the SMC galaxy

M. J. Rickard, R. Hainich, W. -R. Hamann +9

Massive stars are among the main cosmic engines driving the evolution of star-forming galaxies. Their powerful ionising radiation and stellar winds inject a large amount of energy…

astro-ph.SR2022★ 25 cited

The earliest O-type eclipsing binary in the Small Magellanic Cloud, AzV 476: A comprehensive analysis reveals surprisingly low stellar masses

D. Pauli, L. M. Oskinova, W. -R. Hamann +7

Massive stars at low metallicity are among the main feedback agents in the early Universe and in present-day star forming galaxies. When in binaries, these stars are potential prog…

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