R
Radosław Smolec
Researcher at Polish Academy of Sciences
Publications - 158
Citations - 4996
Radosław Smolec is an academic researcher from Polish Academy of Sciences. The author has contributed to research in topics: Stars & Cepheid variable. The author has an hindex of 32, co-authored 148 publications receiving 3933 citations. Previous affiliations of Radosław Smolec include University of Vienna.
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An eclipsing-binary distance to the Large Magellanic Cloud accurate to two per cent
Grzegorz Pietrzyński,Grzegorz Pietrzyński,Dariusz Graczyk,Wolfgang Gieren,Ian B. Thompson,Bogumił Pilecki,Bogumił Pilecki,Andrzej Udalski,Igor Soszyński,Szymon Kozłowski,Piotr Konorski,Ksenia Suchomska,Giuseppe Bono,Giuseppe Bono,P. G. Prada Moroni,Sandro Villanova,Nicolas Nardetto,F. Bresolin,R. P. Kudritzki,Jesper Storm,Alexandre Gallenne,Radosław Smolec,Dante Minniti,M. Kubiak,Michał K. Szymański,Radosław Poleski,Radosław Poleski,Łukasz Wyrzykowski,Krzysztof Ulaczyk,P. Pietrukowicz,Marek Górski,Paulina Karczmarek +31 more
TL;DR: Determinations of the distances to eight long-period, late-type eclipsing systems in the Large Magellanic Cloud, composed of cool, giant stars, provide a firm base for a 3-per-cent determination of the Hubble constant.
Journal ArticleDOI
Modules for Experiments in Stellar Astrophysics (MESA): Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation
Bill Paxton,Radosław Smolec,Josiah Schwab,A. Gautschy,Lars Bildsten,Lars Bildsten,Matteo Cantiello,Matteo Cantiello,Aaron Dotter,Robert Farmer,Jared A. Goldberg,Adam S. Jermyn,Shashi M. Kanbur,Pablo Marchant,Anne Thoul,Richard H. D. Townsend,William M. Wolf,William M. Wolf,Michael Zhang,Francis Timmes +19 more
TL;DR: In this paper, the capabilities of the open-knowledge software instrument Modules for Experiments in Stellar Astrophysics (MESA) have been updated to improve numerical energy conservation capabilities, including during mass changes.
Journal ArticleDOI
Modules for Experiments in Stellar Astrophysics (MESA): Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation
Bill Paxton,Radosław Smolec,Josiah Schwab,A. Gautschy,Lars Bildsten,Lars Bildsten,Matteo Cantiello,Matteo Cantiello,Aaron Dotter,Robert Farmer,Jared A. Goldberg,Adam S. Jermyn,Shashi M. Kanbur,Pablo Marchant,Anne Thoul,Richard H. D. Townsend,William M. Wolf,William M. Wolf,Michael Zhang,Francis Timmes +19 more
TL;DR: In this article, the capabilities of the open-knowledge software instrument Modules for Experiments in Stellar Astrophysics (MESA) have been updated to improve numerical energy conservation capabilities, including during mass changes.
Journal ArticleDOI
A distance to the Large Magellanic Cloud that is precise to one per cent.
Grzegorz Pietrzyński,Dariusz Graczyk,Dariusz Graczyk,Alexandre Gallenne,Alexandre Gallenne,Wolfgang Gieren,Ian B. Thompson,Bogumił Pilecki,Paulina Karczmarek,Marek Górski,K. Suchomska,Mónica Taormina,Bartłomiej Zgirski,P. Wielgórski,Z. Kołaczkowski,Piotr Konorski,Sandro Villanova,Nicolas Nardetto,Pierre Kervella,Fabio Bresolin,Rolf-Peter Kudritzki,Jesper Storm,Radosław Smolec,W. Narloch +23 more
TL;DR: A new calibration of the surface brightness–colour relation of eclipsing binary stars gives a distance to the Large Magellanic Cloud that is precise to one per cent.
Journal ArticleDOI
A distance to the Large Magellanic Cloud that is precise to one per cent
Grzegorz Pietrzyński,Dariusz Graczyk,Dariusz Graczyk,Alexandre Gallenne,Alexandre Gallenne,Wolfgang Gieren,Ian B. Thompson,Bogumił Pilecki,Paulina Karczmarek,Marek Górski,K. Suchomska,Mónica Taormina,Bartłomiej Zgirski,P. Wielgórski,Z. Kołaczkowski,Piotr Konorski,Sandro Villanova,Nicolas Nardetto,Pierre Kervella,Fabio Bresolin,Rolf-Peter Kudritzki,Jesper Storm,Radosław Smolec,W. Narloch +23 more
TL;DR: In this article, a new calibration of the surface brightness-colour relation of eclipsing binary stars gives a distance to the Large Magellanic Cloud that is precise to one per cent.