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V. Shevchenko

3 papers hereh-index 10557 citations91 works total

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

author position
  • middle author2
  • last author1

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph3
same name
  • V. Shevchenko — 83 papers, h 80
  • V. Shevchenko — 61 papers
  • V. Shevchenko — 14 papers, h 11
  • V. Shevchenko — 10 papers
  • V. Shevchenko — 10 papers, h 25
  • V. Shevchenko — 8 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
20012006
most citedResults of the ROTOR-program. I. The long-term photometric variability of classical T Tauri stars

193 citations · 260 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph2006★ 193 cited

Results of the ROTOR-program. I. The long-term photometric variability of classical T Tauri stars

K. N. Grankin, S. Yu. Melnikov, J. Bouvier +2

We present a unique, homogeneous database of photometric measurements for Classical T Tauri stars extending up to 20 years. The database contains more than 21,000 UBVR observations…

astro-ph2004★ 47 cited

The Stellar Composition of the Star Formation Region CMa R1 -- III. A new outburst of the Be star component in Z CMa

M. E. van den Ancker, P. F. C. Blondel, H. R. E. Tjin A Djie +5

We report on a recent event in which, after more than a decade of slowly fading, the visual brightness of the massive young binary Z CMa suddenly started to rise by about 1 magnitu…

astro-ph2001★ 20 cited

The Stellar Composition of the Star Formation Region CMa R1. II. Spectroscopic and Photometric Observations of 9 Young Stars

H. R. E. Tjin A Djie, M. E. van den Ancker, P. F. C. Blondel +4

We present new high and low resolution spectroscopic and photometric data of nine members of the young association CMa R1. All the stars have circumstellar dust at some distance as…

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