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R Leonis

|caption=Location of R Leonis (circled) }}

| dec= | appmag_v = 4.4 - 11.3 }} | r-i = | v-r = | b-v = 1.26 | u-b = | variable = Mira variable }} | dist_ly = 372 | dist_pc = 114 }} 350 | luminosity = 3,537 | temperature = 2,9303,080 }}

}}

R Leonis is a red giant Mira-type variable star located approximately 370 light years away in the constellation Leo.

The apparent magnitude of R Leonis varies between 4.31 and 11.65 with a period of 312 days. At maximum it can be seen with the naked eye, while at minimum a telescope of at least 7 cm is needed. The star's effective temperature is estimated to be 2,9303,080kelvins and radius spans , roughly Mars's orbital zone. Provided by Wikipedia
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    Quality assurance in RT-PCR-based BCR/ABL diagnostics - results of an interlaboratory test and a standardization approach by Burmeister, Thomas (Author) , Maurer, J. (Author) , Aivado, M. (Author) , Elmaagacli, A. H. (Author) , Grünebach, F. (Author) , Held, K. R. (Author) , Heß, G. (Author) , Hochhaus, Andreas (Author) , Höppner, W. (Author) , Lentes, K. U. (Author) , Lübbert, M. (Author) , Schäfer, K. L. (Author) , Schafhausen, P. (Author) , Schmidt, C. A. (Author) , Schüler, F. (Author) , Seeger, K. (Author) , Seelig, R. (Author) , Thiede, C. (Author) , Viehmann, S. (Author) , Weber, C. (Author) , Wilhelm, S. (Author) , Christmann, A. (Author) , Clement, J. H. (Author) , Ebener, U. (Author) , Enczmann, J. (Author) , Leo, R. (Author) , Schleuning, M. (Author) , Schoch, R. (Author) , Thiel, E. (Author) ,


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