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Bychkov, V. D. ; Bychkova, L. V. ; Madej, J. (2008)
  • Publisher: Odessa I.I.Mechnikov National University< RSI "Astronomical Observatory"
  • Journal: Odessa Astronomical Publications (issn: 1810-4215, eissn: 1810-4215)
  • Subject: Stars; magnetic fields of stars; basic properties
    arxiv: Astrophysics::Galaxy Astrophysics | Astrophysics::Cosmology and Extragalactic Astrophysics | Astrophysics::Earth and Planetary Astrophysics | Astrophysics::Solar and Stellar Astrophysics

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.
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