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A. Miroshnichenko

18 papers hereh-index 399 citations25 works total

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

author position
  • first author2
  • middle author11
  • last author1

Across the 14 of 18 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR17
  • astro-ph1
same name
  • A. Miroshnichenko — 108 papers, h 77
  • A. Miroshnichenko — 32 papers, h 21
  • A. Miroshnichenko — 12 papers, h 7
  • A. Miroshnichenko — 4 papers, h 3
  • A. Miroshnichenko — 2 papers, h 8
  • A. Miroshnichenko — 1 paper, h 1

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
20062026
most citedProperties of the δ Scorpii Circumstellar Disk from Continuum Modeling

63 citations · 298 across the 18 of their papers we have counts for

collaborators
Showing 2013Show all

3 papers · 1 filter

astro-ph.SR2013★ 18 cited

TYC 3159-6-1: a runaway blue supergiant

V. V. Gvaramadze, A. S. Miroshnichenko, N. Castro +2

We report the results of optical spectroscopy of a candidate evolved massive star in the Cygnus X region, TYC 3159-6-1, revealed via detection of its curious circumstellar nebula i…

astro-ph.SR2013★ 31 cited

Doppler tomography of the circumstellar disk of π Aquarii

S. V. Zharikov, A. S. Miroshnichenko, E. Pollmann +17

The work is aimed at a study of the circumstellar disk of the bright classical binary Be star π Aqr. We analysed variations of a double-peaked profile of the Hα emission line in th…

astro-ph.SR2013

BG Gem - a Poorly-Studied Binary with a Possible Black Hole Component

N. A. Drake, A. S. Miroshnichenko, S. Danford +1

BG Gem is an eclipsing binary with a 91.6-day orbital period. The more massive primary component does not seem to show absorption lines in the spectrum, while the less massive seco…

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