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K. Stoyanov

55 papers hereh-index 10408 citations83 works total

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

author position
  • first author7
  • middle author32
  • last author10

Across the 49 of 55 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR50
  • astro-ph.HE2
  • astro-ph1
  • astro-ph.CO1
  • astro-ph.GA1
same name
  • K. Stoyanov — 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
20082026
most citedThe awakening of BL Lacertae: observations by Fermi, Swift, and the GASP-WEBT

135 citations · 536 across the 55 of their papers we have counts for

collaborators
Showing 2016Show all

4 papers · 1 filter

astro-ph.SR2016★ 2 cited

The cataclysmic variable AE Aquarii: B-V colour of the flares

R. K. Zamanov, G. Y. Latev, S. Boeva +3

We report simultaneous observations of the flaring behaviour of the cataclysmic variable star AE Aqr. The observations are in Johnson B and V bands. The colour-magnitude diagrams (…

astro-ph.SR2016★ 18 cited

AG Pegasi - now a classical symbiotic star in outburst?

T. V. Tomov, K. A. Stoyanov, R. K. Zamanov

Optical spectroscopy study of the recent AG Peg outburst observed during the second half of 2015 is presented. Considerable variations of the intensity and the shape of the spectra…

astro-ph.SR2016★ 34 cited

Active phases and flickering of a symbiotic recurrent nova T CrB

Krystian Ilkiewicz, Joanna Mikolajewska, Kiril Stoyanov +2

T CrB is a symbiotic recurrent nova known to exhibit active phases, characterised by apparent increases in the hot component temperature and the appearance of flickering, i.e. chan…

astro-ph.SR2016★ 21 cited

Optical spectroscopy of Be/gamma-ray binaries

R. K. Zamanov, K. A. Stoyanov, J. Marti +4

We report optical spectroscopic observations of the Be/gamma-ray binaries LSI+61303, MWC 148 and MWC 656. The peak separation and equivalent widths of prominent emission lines (H-a…

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