University of Bahrain
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Statistical magnitude analysis and distance determination of the nearby GOV stars

Show simple item record Sharaf, M.A. 2018-07-22T09:13:09Z 2018-07-22T09:13:09Z 2006-01-01
dc.identifier.issn 1815-3852
dc.description.abstract The present paper has three folds: first, to provide some basic descriptive statistical parameters for the apparent and absolute magnitudes of the nearby stars of spectral type GOV stars Second, to establish the frequency functions o(m) and W(m) of the absolute and apparent magnitudes for these stars. Third , to compute the distance r of these stars as a system assuming that they scatter around a mean absolute magnitude in a Gaussian distribution. The accuracy of the numerical results is satisfactory in that, the percentage error between r and the mean value is less than 3%. en_US
dc.language.iso en en_US
dc.publisher University of Bahrain en_US
dc.rights Attribution-NonCommercial-ShareAlike 4.0 International *
dc.rights.uri *
dc.subject Distance determinations en_US
dc.subject spectral types en_US
dc.subject frequency functions en_US
dc.subject statistical magnitude analysis en_US
dc.title Statistical magnitude analysis and distance determination of the nearby GOV stars en_US
dc.type Article en_US
dc.source.title Arab Journal of Basic and Applied Sciences
dc.abbreviatedsourcetitle AJBAS

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