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researcher

S. Stefanov

4 papers hereh-index 28 citations8 works total

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

author position
  • middle author1
  • last author3

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR3
  • astro-ph.EP1
same name
  • S. Stefanov — 7 papers, h 2
  • S. Stefanov — 4 papers, h 2
  • S. Stefanov — 2 papers, h 2
  • S. Stefanov — 1 paper, h 2
  • S. Stefanov — 1 paper, h 10

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
20212026
most citedH-alpha spectroscopy of the recurrent nova RS Oph during the 2021 outburst

3 citations · 4 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.SR2026

H_alpha observations of the Be/X-ray binary MWC 656

R. Zamanov, V. Marchev, K. A. Stoyanov +8

Context. MWC 656 is a Be/X-ray binary identified as an emission-line object, X-ray and radio source and might be a weak gamma-ray source, harbouring an enigmatic secondary componen…

astro-ph.EP2026

A Warm Massive Pair of Planets around TOI-1232 Revealed with Transit-timing Variations and Doppler Spectroscopy

Deyan P. Mihaylov, Jan Eberhardt, Trifon Trifonov +32

TOI-1232 is a G-dwarf star with a mass of 1.06−0.06+0.07​M⊙​, a radius of 1.07±0.05R⊙​, and slightly higher metallicity than solar of Fe/H = 0.18±0.05.…

astro-ph.SR2024★ 1 cited

Size of the accretion disc in the recurrent nova T CrB

R. K. Zamanov, K. A. Stoyanov, V. Marchev +7

We present high resolution (0.06 A/px) spectroscopic observations of the recurrent nova T Coronae Borealis obtained during the last 1.5 years (September 2022 -- January 2024), with…

astro-ph.SR2021★ 3 cited

H-alpha spectroscopy of the recurrent nova RS Oph during the 2021 outburst

R. K. Zamanov, K. A. Stoyanov, Y. M. Nikolov +3

We report spectroscopic observations of the Hα emission line of the recurrent nova RS~Oph obtained between 12 and 23 August 2021 during the recent outburst. On the basis of the s…

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