publication . Article . 2008


V. D. Bychkov; L. V. Bychkova; J. Madej;
Open Access English
  • Published: 01 Dec 2008 Journal: Odessa Astronomical Publications (issn: 1810-4215, eissn: 1810-4215, Copyright policy)
  • Publisher: Odessa I.I.Mechnikov National University< RSI "Astronomical Observatory"
Now it is known about 1212 stars of the main sequence and giants (from them 610 stars - it is chemically peculiarity (CP) stars) for which direct measurements of magnetic fields were spent (Bychkov et al.,2008). Let's consider, what representations were generated about magnetic fields (MT) of stars on the basis of available observations data.
Persistent Identifiers
arXiv: Astrophysics::Galaxy AstrophysicsAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics
free text keywords: Stars; magnetic fields of stars; basic properties, lcsh:Astronomy, lcsh:QB1-991
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