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researcher

M. Burlak

34 papers hereh-index 9316 citations109 works total

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

author position
  • sole author1
  • first author5
  • middle author24
  • last author2

Across the 32 of 34 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR26
  • astro-ph.HE4
  • astro-ph.GA3
  • astro-ph1
same name
  • M. Burlak — 5 papers, h 3
  • M. Burlak — 3 papers, h 2
  • M. Burlak — 1 paper

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
20072026
most citedA flare in the optical spotted in the changing-look Seyfert NGC 3516

31 citations · 76 across the 23 of their papers we have counts for

collaborators
Showing 2026Show all

4 papers · 1 filter

astro-ph.SR2026

Photometric and spectral variability of the candidate post-AGB star IRAS 07506-0345

N. P. Ikonnikova, M. A. Burlak, A. V. Dodin

We report photometric and spectroscopic observations of the poorly studied post-AGB candidate IRAS 07506-0345, obtained with the telescopes of the Caucasian Mountain Observatory of…

astro-ph.SR2026

The curved jet in the young star FN Tau

M. A. Burlak, A. V. Dodin, A. V. Zharova +5

In the vicinity of the young star FN Tau, we have detected a microjet and four Herbig-Haro objects, whose positions and kinematics indicate the presence of a bipolar collimated out…

astro-ph.SR2026

Photometric and Spectral Evolution of the Symbiotic Nova HM Sagittae since 2003

N. P. Ikonnikova, V. I. Shenavrin, G. V. Komissarova +2

We present photometric and spectral monitoring of the symbiotic system HM Sge, which consists of a Mira variable with a dust shell and a hot white dwarf ionizing the surrounding ga…

astro-ph.SR2026

The eruptive young star IRAS 21204+4913

M. A. Burlak, A. V. Dodin, A. V. Zharova +7

The results of photometric, polarimetric, and spectroscopic observations are presented for the young star IRAS 21204+4913, whose visible brightness has increased by $\approx 5^{\rm…

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