Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Copernicus Astronomical Center, Warsaw
CAMK, Poland
N. Copernicus Astronomical Center, Poland
Copernicus Astronomical Center, Warsaw, Poland
N. Copernicus Astronomical Center, Warsaw, Poland
Nicolaus Copernicus Astronomical Center, Warsaw, Poland
Copernicus Astronomical Center,Warsaw, Pl
Copernicus Astrononmical Center, Poland
Copernicus Center
N.Copernicus Astronomical Center Poland
N.Copernicus Astr. Center, Warsaw, Poland
Observatoire de Paris, Meudon, France
Observatoire de Paris, France
Copernicus Astronomical Center, Bartycka 18, 00-716 Warsaw, Poland Akademia Nauk, Centrum Astronomiczne, Warsaw, Poland
Scuola Internazionale Superiore di Studi Avanzati, Trieste, Italy; Leicester, University, England
NCAC-Warsaw, Poland
Copernicus Astronomical Center, ul. Bartycka 18, 00-716 Warsaw, Poland
N. Copernicus Astronomical Center, Warsawa, Poland
Nicolaus Copernicus Astronomical Center, 00 716 Warsaw, Poland
Nicolaus Copernicus Astronomical Center, Bartycka 18, 00-716 Warsaw, Poland
CAMK
Polish Academy of Sciences, Astronomical Center, Warsaw, Poland
Copernicus Astronomical Center, Bartycka 18, PL-00-716 Warsaw, Poland
CAMK, Centum Astronomiczne im. Mikolaja Kopernika
Southampton Univ., England
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA
Leicester, University, England
Copernicus Astronomical Center, Bartycka 18, 00-716 Warsaw, Poland
Polish Academy of Sciences, Astronomical Centre, Warsaw, Poland
N. Copernicus Astronomical Center, Bartycka 18, 00-716 Warsaw, Poland
N. Copernicus Astronomical Center
Copernicus Astronomical Center PAS
N.Copernicus Astronomical Center, Poland
Copernicus Astronomical Center, PAS
Harvard-Smithsonian Center for Astrophysics, Cambrid
"Postępy Astronomii" - a popular quarterly astronomical journal
A cloud model of active galactic nuclei: the iron K-alpha line diagnostics
Absorption spectrum of the quasar HS1603+3820 I. Observations and data analysis
Accreting corona model of the X-ray variability in soft state GBH and AGN
Accreting corona model of the X-ray variability in soft state X-ray binaries and active galactic nuclei
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