... M., Supernovae and Supernovae Remnants , IAJ , 1978, 13(7/8), 267. de Groot, M ... M., (editor), Ernst Julius , 1893-1985, The Man and the Scientist , IAJ , 1986, 17(4 ...
92. http://star.arm.ac.uk/preprints/2011/589.pdf
... have tested negative for co-orbital motion within the perio d [ - 106 yr, 106 yr ... Cellino, A., Capaccioni, F., Capria, M. T., de Sanctis, M. C., Keller, H. U ... R. A., Keesey, M. S., Lieske, J. H., Ostro, S. J., Standish E. M., Wimberly, R. N ...
93. http://star.arm.ac.uk/preprints/2015/687.pdf
... M. J., 2006, A&A, 454, 571 Alecian G., Stift M. J., Dorfi E. A., 2011, MNRAS, 418, 986 Bab el J., Michaud G., 1991, A&A, 248, 155 Bischof K. M., 2005, Memorie della Societa Astronomica Italiana Supplementi, 8, 64 Chandrasekhar S., 1935, MNRAS, 96, 21 ...
94. http://star.arm.ac.uk/preprints/451.pdf
... 2 , C.M. Johns-Krull3 , J.G. Doyle1 , I. Ugarte-Urra1 , M.S. Madjarska1, Butler1 1 2 ... M., & Falciani, R. 1982, A&AS, 47, 485 Allen, C. W. 1976, Astrophysical Quantities ...
95. http://star.arm.ac.uk/preprints/2010/571b.pdf
... 102 104 102 104 105 106 106 106 106 106 106 107 106 106 106 106 106 108 tss , 2.09 в ... M.J. & Benz, A.O. 1988 ApJ, 332, 447 Aschwanden, M.J. 1990, A&AS, 85, 1141 Berger, E ...
96. http://star.arm.ac.uk/preprints/441.pdf
... 1995, Sol. Phys., 162, 129 Summers, H.P. & Hooper, M.B., 1983, Plasma Physics, 25, 1311 Teriaca, L., Madjarska, M.S. & Doyle, J.G., 2001, Sol. ...
97. http://star.arm.ac.uk/preprints/454.pdf
... M a = 10 M a = 30 0.27943 0.30069 0.32986 0.35788 0.38442 0.23392 0.25072 0.26344 0 ... M a = 10 M a = 30 0.24811 0.26937 0.29198 0.31426 0.33806 0.19424 0.21581 0.22668 0 ...
98. http://star.arm.ac.uk/preprints/402.ps
... m] Na Nd S1 1 { 0 S(9) 1.6873 0.025 0.014 0.035 1 { 0 S(8) 1.7143 < 0.015 0.012 0.026 1 { 0 S(7) 1.7475 0.097 0.093 0.144 1 { 0 S(6) 1.7876 0.063 0.061 0.090 1 { 0 S(5) 1.8353 0.261 0.293 0.322 1 { 0 S(4) 1.8914 0.099 0.109 0.351 1 { 0 S(2) 2.0332 0.328 0 ...
99. http://star.arm.ac.uk/~ambn/300csj.ps
... mљ A) H i fl 4340.4 60 3.41 bl S iii 4 ffi 4101.7 34 3.40 bl Si iii 8;10 ffl 3970.1 63 2.90 bl C ii 38 3.24 \Sigma 0.29 C ii Yan 87 12.01 4637.4 55 1.237 2.37 12.02 4306.3 27 1.678 2.33 17.08 4802.7 134 0.411 2.46 28 4313.1 95 0.378 2.44 4323.1 26 1 ...
100. http://star.arm.ac.uk/preprints/2012/618.pdf
... Each peak of luminosity is about 106 L and the energy released causes the radius to increase, leading the star to evolve to ... About eight flashes after 3 ignition, accretion stops (M = 0.8 M )and the merged star attains aradius of 18 R . ...