Projects funded by the NCN

Classical pulsators through diverse stellar systems: contrast between pulsation modes

Call: OPUS 9 , Panel: ST9

Principal investigator: dr hab. Radosław Smolec

Centrum Astronomiczne im. Mikołaja Kopernika PAN

Determination of physical parameters of type II Cepheids in eclipsing binary systems.

Call: SONATA 8 , Panel: ST9

Principal investigator: dr Bogumił Pilecki

Centrum Astronomiczne im. Mikołaja Kopernika PAN

Cepheids in binary systems as a unique laboratory for calibration of the cosmic distance scale and studying theories of ...

Call: MAESTRO 3 , Panel: ST9

Principal investigator: prof. Grzegorz Pietrzyński

Centrum Astronomiczne im. Mikołaja Kopernika PAN

Multi-mode, non-radial and modulated pulsation of RR Lyrae stars and Cepheids

Call: OPUS 3 , Panel: ST9

Principal investigator: dr Radosław Smolec

Centrum Astronomiczne im. Mikołaja Kopernika PAN

Towards understanding of low-amplitude variability of classical Cepheids

Call: OPUS 27 , Panel: ST9

Principal investigator: dr hab. Radosław Smolec

Centrum Astronomiczne im. Mikołaja Kopernika PAN

Understanding Cepheids: physical and empirical basis for our main tool for distance determination in the Universe.

Call: SONATA BIS 10 , Panel: ST9

Principal investigator: dr Bogumił Ferdynand Pilecki

Centrum Astronomiczne im. Mikołaja Kopernika PAN

Type II Cepheids as Precision Distance Indicators

Call: PRELUDIUM 16 , Panel: ST9

Principal investigator: Piotr Wielgórski

Centrum Astronomiczne im. Mikołaja Kopernika PAN

Classical Cepheids as testbeds for stellar evolution and pulsation theories

Call: SONATA BIS 8 , Panel: ST9

Principal investigator: dr hab. Radosław Smolec

Centrum Astronomiczne im. Mikołaja Kopernika PAN

Precise and accurate measurement of the Hubble Constant in the era of Gaia

Call: MAESTRO 9 , Panel: ST9

Principal investigator: prof. Grzegorz Pietrzyński

Centrum Astronomiczne im. Mikołaja Kopernika PAN

Imaging of the Galaxy with pulsating stars

Call: MAESTRO 8 , Panel: ST9

Principal investigator: prof. Igor Soszyński

Uniwersytet Warszawski, Wydział Fizyki