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researcher

P. Bezák

3 papers hereh-index 172.5k citations48 works total

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

author position
  • middle author1
  • last author2

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

fields
  • astro-ph.GA1
  • astro-ph.HE1
  • astro-ph.SR1
same name
  • P. Bezák — 2 papers, h 7

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
20212024
most citedThe Super-Soft Source Phase of the recurrent nova V3890 Sgr

18 citations · 26 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2024★ 1 cited

Searching for similarities in the accretion flow of Seyfert 1 galaxies and cataclysmic variables based on flare profiles of IRAS 13224-3809, 1H 0707-495, Mrk 766 and MV Lyr

A. Dobrotka, H. Negoro, P. Bezak

AIMS: We studied fast variability of three selected AGNs, IRAS 13224-3809, 1H 0707-495 and Mrk 766, and the cataclysmic variable MV Lyr observed by XMM-Newton and Kepler spacecraft…

astro-ph.SR2023★ 7 cited

Recurrent mini-outbursts and a magnetic white dwarf in the symbiotic system FN Sgr

J. Magdolen, A. Dobrotka, M. Orio +5

AIMS: We investigated the optical variability of the symbiotic binary FN Sgr, with photometric monitoring during ≃55 years and with a high-cadence Kepler light curve lasting…

astro-ph.HE2021★ 18 cited

The Super-Soft Source Phase of the recurrent nova V3890 Sgr

J. -U. Ness, A. P. Beardmore, P. Bezak +9

The 30-year recurrent symbiotic nova V3890 Sgr exploded 2019 August 28 and was observed with multiple X-ray telescopes. An XMM-Newton observation during the SSS phase captured a hi…

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