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researcher

N. Petrov

9 papers hereh-index 7144 citations42 works total

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

author position
  • middle author2
  • last author5

Across the 7 of 9 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR6
  • astro-ph.GA3
same name
  • N. Petrov — 10 papers, h 19
  • N. Petrov — 9 papers, h 10
  • N. Petrov — 7 papers, h 10
  • N. Petrov — 4 papers, h 21
  • N. Petrov — 3 papers, h 11
  • N. Petrov — 3 papers, h 0

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
20132022
most citedThe W UMa binaries USNO-A2.0 1350-17365531, V471 Cas, V479 Lac and V560 Lac: light curve solutions and global parameters based on the GAIA distances

20 citations · 68 across the 9 of their papers we have counts for

collaborators
Showing 2018Show all

3 papers · 1 filter

astro-ph.SR2018★ 12 cited

Spectral observations of X Persei: Connection between H-alpha and X-ray emission

R. Zamanov, K. A. Stoyanov, U. Wolter +2

We present spectroscopic observations of the Be/X-ray binary X Per obtained during the period 1999 - 2018. Using new and published data, we found that during "disc-rise" the expans…

astro-ph.SR2018★ 20 cited

The W UMa binaries USNO-A2.0 1350-17365531, V471 Cas, V479 Lac and V560 Lac: light curve solutions and global parameters based on the GAIA distances

Diana P. Kjurkchieva, Velimir A. Popov, Yordanka Eneva +1

We present photometric observations in Sloan filters g', i' of the eclipsing W UMa stars USNO-A2.0 1350-17365531, V471 Cas, V479 Lac and V560 Lac. The sinusoidal-like O-C diagram o…

astro-ph.SR2018★ 12 cited

NSVS 2569022: a peculiar binary among the W UMa stars with extremely small mass ratios

Diana P. Kjurkchieva, Velimir A. Popov, Nikola I. Petrov

Photometric observations of the W UMa binary NSVS 2569022 are presented. The light curve solution reveals that both components are of F spectral type (temperatures T1​=T2​=6100…

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