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R31 - A massive O + W-R star binary in the Small Magellanic Cloud
Publications of the Astronomical Society of the Pacific, 1984The authors present spectroscopic data on the O6 + WN3 binary R31 in the SMC, which improve the orbital determination of Moffat (1982). The period is found to be 6.538 days. From several considerations they consider an eccentricity of ≡0.2 to be possible.
J. B. Hutchings +3 more
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Thermal stability of R218 (C3F8) and R31-10 (C4F10) under heat exposure
High Temperature, 2015The results of study of the thermal decomposition of fluorocarbons under constant and cyclic heating are presented. Studies are carried out in the temperature range of 500–670°C. For continuous heating, the exposure time was 4 h; up to 106 cycles were carried out under cyclic heating.
R. L. Gerasimov, I. M. Mazurin
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Melrose Project Daily Records, T1N R31 E29
1994Daily records for Tolar Southeast - T1N R31 ...
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Melrose Project Daily Records, T1N R31 E33
1994Daily records for Tolar Southeast - T1N R31 ...
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Melrose Project Daily Records, T1N R31 E28
1994Daily records for Tolar Southeast - T1N R31 ...
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Melrose Project Daily Records, T1N R31 E34
1993Daily records for Tolar Southeast - T1N R31 ...
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Melrose Project Daily Records, T1N R31 E21
1994Daily records for Tolar Southeast - T1N R31 ...
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Melrose Project Daily Records, T1N R31 E25
1994Daily records for Tolar Southeast - T1N R31 ...
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The Backlund’s theorem in Minkowski 3-space R31
Applied Mathematics and Computation, 2005zbMATH Open Web Interface contents unavailable due to conflicting licenses.
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Melrose Project Daily Records, T1N R31 E27
1994Daily records for Tolar Southeast - T1N R31 ...
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