RW Tri – its Negative Superhumps and System Parameters. (arXiv:1902.07502v1 [astro-ph.SR])

RW Tri – its Negative Superhumps and System Parameters. (arXiv:1902.07502v1 [astro-ph.SR])
<a href="http://arxiv.org/find/astro-ph/1/au:+Smak_J/0/1/0/all/0/1">J. Smak</a>

Negative superhumps are detected in the light curves of RW Tri collected in
September 1994 (Smak 1995) and November/December 1957 (Walker 1963). New system
parameters, obtained using $K_2$ and $V_{2,rot}sin i$ (from Poole et al. 2003)
and $q$ (estimated from $P_{nSH}$), are $M_1=0.60pm 0.20Modot$, $M_2=0.48pm
0.15Modot$, $A=1.13pm 0.09times 10^{11}$cm and $i=72.5pm 2.5$.

Negative superhumps are detected in the light curves of RW Tri collected in
September 1994 (Smak 1995) and November/December 1957 (Walker 1963). New system
parameters, obtained using $K_2$ and $V_{2,rot}sin i$ (from Poole et al. 2003)
and $q$ (estimated from $P_{nSH}$), are $M_1=0.60pm 0.20Modot$, $M_2=0.48pm
0.15Modot$, $A=1.13pm 0.09times 10^{11}$cm and $i=72.5pm 2.5$.

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