'Ap stars' diaporamas de présentation

Notes:

Notes: In many of the Fourier transforms the frequency is given in c/d = cycles per day. To convert to m Hz multiply numbers by 11.57 HD 101065 has a period of ~12 minutes. If you use Period04 on the data this corresponds to ~118 c/d. Rapidly Oscillating Peculiar Magnetic A stars.

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Peculiar A Stars

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ATOMIC DATA AND ELECTRON-IMPACT BROADENING OF SPECTRAL LINES OF RARE EARTHS

ATOMIC DATA AND ELECTRON-IMPACT BROADENING OF SPECTRAL LINES OF RARE EARTHS. Zoran Simi? and Milan S. Dimitrijevi? Astronomical Observatory, Volgina 7, 11060 Belgrade, Serbia zsimic@aob.bg.ac.rs; mdimitrijevic@aob.bg.ac.rs. Motivation.

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ATOMIC DATA AND ELECTRON-IMPACT BROADENING OF SPECTRAL LINES OF RARE EARTHS

ATOMIC DATA AND ELECTRON-IMPACT BROADENING OF SPECTRAL LINES OF RARE EARTHS. Zoran Simi? and Milan S. Dimitrijevi? Astronomical Observatory, Volgina 7, 11060 Belgrade, Serbia zsimic@aob.bg.ac.rs; mdimitrijevic@aob.bg.ac.rs. Motivation.

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Magneto-rotational instability in the solar core and Ap star envelopes

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Magneto-rotational instability in the solar core and Ap star envelopes

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Writing an Observing Proposal

Writing an Observing Proposal. Writing a good observing proposal is challenging because:. You have a committee (many judges) The judges are often not experts in your field

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