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pro vyhledávání: '"Panagi, P. M."'
We present statistically robust observational evidence which imposes new limits on dynamo saturation in young solar-type stars. These are inferred from the increasing amplitude of the V-band optical flux with rotation, caused by the filling of the di
Externí odkaz:
http://arxiv.org/abs/astro-ph/9409023
Autor:
Byrne, P. B., Panagi, P. M., Alessandro Lanzafame, Avgoloupis, S., Huenemoerder, D. P., Kilkenny, D., Marang, F., Panov, K. P., Roberts, G., Seiradakis, J. H., Vanwyk, F.
Publikováno v:
ResearcherID
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::97289fdc2f7d3ffabf36cfdfd606b8ce
http://hdl.handle.net/20.500.11769/44085
http://hdl.handle.net/20.500.11769/44085