Projects funded by the NCN
Metallicity of HADS and SX Phoenicis stars.
2019/33/N/ST9/01818
Keywords:
HADS stars SX Phoenicis stars variable stars metallicity stellar evolution stellar populations
Descriptors:
- ST9_7: Stars and stellar systems
- ST9_17: Large data bases: archiving, handling and analysis
Panel:
ST9 - Astronomy and space science: astrophysics, astrochemistry, astrobiology, solar system, planetary systems, stellar, galactic and extragalactic astronomy, space science, instrumentation
Host institution :
Uniwersytet Wrocławski, Wydział Fizyki i Astronomii
woj.
Principal investigator (from the host institution):
Number of co-investigators in the project: 2
Call: PRELUDIUM 17 - announced on 2019-03-15
Amount awarded: 131 900 PLN
Project start date (Y-m-d): 2020-02-25
Project end date (Y-m-d): 2023-08-24
Project duration:: 42 months (the same as in the proposal)
Project status: Project settled
Project description
Download the project description in a pdf file
Note - project descriptions were prepared by the authors of the applications themselves and placed in the system in an unchanged form.
Information in the final report
- Publication in academic press/journals (1)
- HD133729: A blue large-amplitude pulsator in orbit around a main-sequence B-type starAuthors:Pigulski A., Kotysz K., Kołaczek-Szymański P.A.Academic press:Astronomy & Astrophysics (rok: 2022, tom: 663, A62, strony: 45667), Wydawca: EDP SciencesStatus:PublishedDOI:10.1051/0004-6361/202243293 - link to the publication