Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Torun Centre for Astronomy, Nicolaus Copernicus University
N. Copernicus Univesity, Torun, Poland
Torun Centre for Astronomy, Nicolaus Copernicus University, Poland;
Torun CfA, Poland
Torun Centre for Astronomy in Poland
Toruń Centre for Astronomy, Nicolaus Copernicus University, Poland
Toruń Centre for Astronomy, Nicolaus Copernicus University, ul. Gagarina 11, 87100 Toruń, Poland
Toruń Centre for Astronomy, Nicolaus Copernicus University, ul. Gagarina 11, PL-87100 Toruń, Poland
Toruri Radio Astronomy Observatory, Nicolaus Copernicus University, ul. Gagarina 11, PL-87100 Toruri, Poland
Torun Centre for Astronomy, Nicolaus Copernicus University, ul. Gagarina 11, PL-87100 Torun, Poland
Obserwatorium Astronomiczne, Torun, Poland
Toruń Centre for Astronomy, Nicolaus Copernicus University, Poland for Astronomy, Nicolaus Copernicus University, Torun, Poland.
Toruń Centre for Astronomy, Nicolaus Copernicus University, Poland s
Toruń Centre for Astronomy, Nicolaus Copernicus University, Gagarina 11, PL-87100 Toruń, Poland
Toruń Centre for Astronomy, Nicolaus Copernicus University, Gagarina 11, 87-100 Toruń, Poland
Torun Radio Astronomy Observatory, Poland
Toruń Centre for Astronomy, Nicolaus Copernicus University, Gagarina 11, 87100 Toruń, Poland
Torun, Obserwatorium Astronomiczne, Poland
Torun Centre for Astronomy, Nicolaus Copernicus University, Gagarina 11, 87-100 Toruń, Poland
Torun Centre for Astronomy, Nicolaus Copernicus University, Torun, Poland
Centre for Astronomy, Nicolaus Copernicus University, Gagarina 11, Torun, Poland
6.7 GHz methanol masers at sites of star formation. A blind survey of the Galactic plane between 20 degr <<= 40 degr and |b| <= 0\fdg52
6.7GHz methanol maser emission survey (Szymczak+, 2000)
A comparison of OH and H_2O maser properties of Mira and semiregular variable stars
A multi-transition molecular line study of candidate massive young stellar objects associated with methanol masers
A search for observational evidence of OH molecule photoproduction
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Profile ID: LFWR-SCP-P-5328