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researcher

M. Górski

14 papers hereh-index 8846 citations14 works total

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

author position
  • first author1
  • middle author11

Across the 12 of 14 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR8
  • astro-ph.GA5
  • astro-ph.CO1
same name
  • M. Górski — 548 papers
  • M. Górski — 28 papers, h 0
  • M. Górski — 23 papers, h 20
  • M. Górski — 3 papers, h 2
  • M. Górski — 2 papers, h 1
  • M. Górski — 1 paper, h 4

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
20132021
most citedThe Araucaria Project. The distance to the Small Magellanic Cloud from late-type eclipsing binaries

235 citations · 588 across the 14 of their papers we have counts for

collaborators
Showing 2019Show all

3 papers · 1 filter

astro-ph.SR2019★ 9 cited

Towards early-type eclipsing binaries as extragalactic milestones: I. Physical parameters of OGLE-LMC-ECL-22270 and OGLE-LMC-ECL-06782

Mónica Taormina, G. Pietrzyński, B. Pilecki +11

In this first paper of the series we describe our project to calibrate the distance determination method based on early-type binary systems. The final objective is to measure accur…

astro-ph.SR2019★ 8 cited

Candidates for non-pulsating stars located in the Cepheid instability strip in the Large Magellanic Cloud based on Strömgren photometry

W. Narloch, G. Pietrzyński, Z. Kołaczkowski +14

We present candidates for non-pulsating stars lying in the classical Cepheid instability strip based on OGLE photometric maps combined with Strömgren photometry obtained with the 4…

astro-ph.SR2019★ 8 cited

Accurate stellar parameters and distance to two evolved eclipsing binary systems, OGLE-BLG-ECL-123903 and OGLE-BLG-ECL-296596, towards the Galactic bulge

K. Suchomska, D. Graczyk, G. Pietrzyński +15

Aim: Our aim is to obtain high-accuracy measurements of the physical and orbital parameters of two evolved eclipsing binary systems, and to use these measurements to study their ev…

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