... M., Pazzani, V., Simon, T. 1987, A&A, 174, 139 Byrne, P.B. 1993, in ``Physics of Solar and Stellar Coronae'', eds. J.L. Linsky & S. Serio, Kluwer, p. 489 Byrne, P.B., McKay, D. 1990, A&A, 227, 490 Byrne, P.B., Doyle, J.G., Brown, A., Linsky, J.L., Rodon`o ...
... M ) M sdB (adopted) M 2,min parameters of 245 5500.86 ± 0.01 2.3098 ± 0.0003 d -6.3 ... mass of 0.47 M , the minimum mass of the companion (0.21 M ) can be derived from the ...
... J., O'Shea, E. & Banerjee, D., 1998, Solar Phys. 181, 51 Doyle, J.G., van den Oord, G.H.J., O'Shea, E. & Banerjee, D., 1999, A&A 347, 335 Erdelyi, R., De Pontieu, B. & Sarro, L.M., 1999, in Magnetic Fields and solar Processes, Florence, Italy, ESA SP-448 ...
... Date: 26 March 2014 13:51:46 GMT . Hi all, . ѓЉ . 1.ѓ ... I'm sure that Dr Myers will be able to give us some insight into the plans for this ... the Bell Lecture Theatre, Physics Building, Queen's University, Belfast, at 7.30 p.m ...
... et al. 1992) one can infer that these parameters correspond to a M = 1.60 ± 0.05 M star with a fractional age between 0.0 and 0 ... M. M. 1985, MNRAS, 217, 305 Napiwotzki, R., Schoenberner, D., & Wenske, V. 1993, A&A, 268, 653 Pojmanski, G. 2002, Acta ...