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Analysis of a Newly Identified Variable Star In Aquarius
Heath Gibson
After calculating the magnitude of variable N in each image, I plotted this against the Julian time at which it was exposed, deriving a light curve. Table 6 contains the data used to plot the light curves for variable candidate N in figures 4 and 5.
After graphing the first light curve (Figure 4), I observed a noticeable bulge at the bottom of the minimum in the sinusoidal curve. Upon closer inspection, it appeared that there were two minima graphed into the same minimum‹the first minimum seemed to reach its nadir five hundredths of a magnitude higher than the second. In order to test this theory, I doubled the period of the curve to see if the two minima could be separated from each other (the original period was 0.15315 days; doubled, it became 0.3063 days) in a new curve (Figure 5). Although there were not enough data points to fill in the part of the curve in phase 0.6 to 0.7, the necessary information to make an educated guess on the variabležs type was present. On the new light curve, there could be seen two distinct minima separated by half a phase; this indicated that the actual period was 0.3063 days. I determined that between the first and second minimum there was a magnitude difference of 0.04, while the magnitude of the variable at each maximum remained constant.
This light curve suggested a contact binary system‹due to its very short period‹with two stars of roughly the same magnitude. With the help of my mentors, I learned that this eclipsing binary (EB) had properties very similar to a W Urase Majoris (W UMa) EB. Using the Caltech library, I found the light curve of a W UMa-type system located in RZ Tauri and found the curve and period to be almost identical to mine. Like my variable, the W UMa had a short period of seven to eight hours; my variable had a period of 0.3063 days, while RZ Tauri had a period of 0.362 days. The light curves were also very similar, as can be observed in Figures 5 and 6. Figure 5, my light curve, has a difference of 0.04 magnitudes between the first and second minima; the W UMa RZ Tauri EBžs magnitude difference between minima is 0.05. The similarity between these two variables show a considerable possibility that variable N is indeed a W UMa type binary system
Table 6. Table of
magnitudes and times for variable star N as graphed in Figure 5
|
Julian Day |
R |
Regular |
Phase |
Phase |
|
2450000+ |
|
Phase |
Repeat |
Repeat |
|
|
|
|
Add 1 |
Subtract 1 |
|
|
|
|
|
|
|
1475.6504 |
13.52 |
0.2551 |
1.2551 |
-0.7449 |
|
1475.6535 |
13.47 |
0.2450 |
1.2450 |
-0.7550 |
|
1475.6562 |
13.58 |
0.2362 |
1.2362 |
-0.7638 |
|
1475.6593 |
13.51 |
0.2261 |
1.2261 |
-0.7739 |
|
1475.6619 |
13.53 |
0.2176 |
1.2176 |
-0.7824 |
|
1475.6646 |
13.54 |
0.2088 |
1.2088 |
-0.7912 |
|
1475.6672 |
13.62 |
0.2003 |
1.2003 |
-0.7997 |
|
1475.6698 |
13.55 |
0.1918 |
1.1918 |
-0.8082 |
|
1475.6723 |
13.59 |
0.1836 |
1.1836 |
-0.8164 |
|
1475.6748 |
13.59 |
0.1755 |
1.1755 |
-0.8245 |
|
1475.6775 |
13.61 |
0.1667 |
1.1667 |
-0.8333 |
|
1475.6806 |
13.61 |
0.1566 |
1.1566 |
-0.8435 |
|
1475.6832 |
13.61 |
0.1481 |
1.1481 |
-0.8519 |
|
1475.6857 |
13.69 |
0.1399 |
1.1399 |
-0.8601 |
|
1475.6885 |
13.65 |
0.1308 |
1.1308 |
-0.8693 |
|
1475.6910 |
13.64 |
0.1226 |
1.1226 |
-0.8774 |
|
1475.6936 |
13.53 |
0.1141 |
1.1141 |
-0.8859 |
|
1475.6973 |
13.71 |
0.1020 |
1.1020 |
-0.8980 |
|
1475.6998 |
13.73 |
0.0939 |
1.0939 |
-0.9061 |
|
1475.7023 |
13.78 |
0.0857 |
1.0857 |
-0.9143 |
|
1475.7048 |
13.74 |
0.0775 |
1.0775 |
-0.9225 |
|
1475.7075 |
13.86 |
0.0687 |
1.0687 |
-0.9313 |
|
1475.7100 |
13.89 |
0.0606 |
1.0606 |
-0.9394 |
|
1475.7126 |
13.93 |
0.0521 |
1.0521 |
-0.9479 |
|
1475.7151 |
13.97 |
0.0439 |
1.0439 |
-0.9561 |
|
1475.7176 |
14.03 |
0.0358 |
1.0358 |
-0.9643 |
|
1475.7201 |
14.08 |
0.0276 |
1.0276 |
-0.9724 |
|
1475.7230 |
14.04 |
0.0181 |
1.0181 |
-0.9819 |
|
1475.7255 |
14.07 |
0.0100 |
1.0100 |
-0.9900 |
|
1475.7281 |
14.11 |
0.0015 |
1.0015 |
-0.9985 |
|
1475.7356 |
14.07 |
-0.0230 |
0.9770 |
-1.0230 |
|
1475.7382 |
14.01 |
-0.0315 |
0.9685 |
-1.0315 |
|
1475.7407 |
13.96 |
-0.0397 |
0.9603 |
-1.0397 |
|
1475.7433 |
13.93 |
-0.0482 |
0.9518 |
-1.0482 |
|
1475.7458 |
13.87 |
-0.0563 |
0.9437 |
-1.0563 |
|
1475.7511 |
13.80 |
-0.0736 |
0.9264 |
-1.0736 |
|
1475.7536 |
13.72 |
-0.0818 |
0.9182 |
-1.0818 |
|
1475.7585 |
13.70 |
-0.0978 |
0.9022 |
-1.0978 |
|
1475.7686 |
13.63 |
-0.1308 |
0.8693 |
-1.1308 |
|
1475.7711 |
13.60 |
-0.1389 |
0.8611 |
-1.1389 |
|
1475.7736 |
13.64 |
-0.1471 |
0.8529 |
-1.1471 |
|
1475.7763 |
13.60 |
-0.1559 |
0.8441 |
-1.1559 |
|
1475.7788 |
13.59 |
-0.1641 |
0.8360 |
-1.1641 |
|
1475.7813 |
13.55 |
-0.1722 |
0.8278 |
-1.1722 |
|
1475.7841 |
13.58 |
-0.1814 |
0.8186 |
-1.1814 |
|
1475.7865 |
13.56 |
-0.1892 |
0.8108 |
-1.1892 |
|
1475.7890 |
13.55 |
-0.1974 |
0.8026 |
-1.1974 |
|
1475.7918 |
13.64 |
-0.2065 |
0.7935 |
-1.2065 |
|
1475.7943 |
13.59 |
-0.2147 |
0.7853 |
-1.2147 |
|
1475.7969 |
13.54 |
-0.2232 |
0.7769 |
-1.2232 |
|
1475.7993 |
13.53 |
-0.2310 |
0.7690 |
-1.2310 |
|
1475.8018 |
13.55 |
-0.2391 |
0.7609 |
-1.2391 |
|
1475.8043 |
13.53 |
-0.2473 |
0.7527 |
-1.2473 |
|
1476.6259 |
13.83 |
0.5704 |
1.5704 |
-0.4296 |
|
1476.6292 |
13.84 |
0.5596 |
1.5596 |
-0.4404 |
|
1476.6319 |
13.92 |
0.5508 |
1.5508 |
-0.4492 |
|
1476.6346 |
13.98 |
0.5420 |
1.5420 |
-0.4581 |
|
1476.6372 |
14.02 |
0.5335 |
1.5335 |
-0.4665 |
|
1476.6397 |
14.06 |
0.5253 |
1.5253 |
-0.4747 |
|
1476.6427 |
14.10 |
0.5155 |
1.5155 |
-0.4845 |
|
1476.6454 |
14.11 |
0.5067 |
1.5067 |
-0.4933 |
|
1476.6482 |
14.14 |
0.4976 |
1.4976 |
-0.5025 |
|
1476.6508 |
14.13 |
0.4891 |
1.4891 |
-0.5109 |
|
1476.6534 |
14.10 |
0.4806 |
1.4806 |
-0.5194 |
|
1476.6561 |
14.12 |
0.4718 |
1.4718 |
-0.5282 |
|
1476.6586 |
14.04 |
0.4636 |
1.4636 |
-0.5364 |
|
1476.6610 |
13.99 |
0.4558 |
1.4558 |
-0.5442 |
|
1476.6635 |
13.93 |
0.4476 |
1.4476 |
-0.5524 |
|
1476.6661 |
13.86 |
0.4391 |
1.4391 |
-0.5609 |
|
1476.6686 |
13.88 |
0.4310 |
1.4310 |
-0.5691 |
|
1476.6711 |
13.83 |
0.4228 |
1.4228 |
-0.5772 |
|
1476.6736 |
13.83 |
0.4146 |
1.4146 |
-0.5854 |
|
1476.6773 |
13.76 |
0.4026 |
1.4026 |
-0.5975 |
|
1476.6798 |
13.73 |
0.3944 |
1.3944 |
-0.6056 |
|
1476.6823 |
13.73 |
0.3862 |
1.3862 |
-0.6138 |
|
1476.6847 |
13.69 |
0.3784 |
1.3784 |
-0.6216 |
|
1476.6993 |
13.59 |
0.3307 |
1.3307 |
-0.6693 |
|
1476.7018 |
13.59 |
0.3226 |
1.3226 |
-0.6774 |
|
1476.7045 |
13.59 |
0.3137 |
1.3137 |
-0.6863 |
|
1476.7067 |
13.58 |
0.3066 |
1.3066 |
-0.6934 |
|
1476.7095 |
13.57 |
0.2974 |
1.2974 |
-0.7026 |
|
1476.7122 |
13.57 |
0.2886 |
1.2886 |
-0.7114 |
|
1476.7147 |
13.55 |
0.2804 |
1.2804 |
-0.7196 |
|
1476.7172 |
13.57 |
0.2723 |
1.2723 |
-0.7277 |
|
1476.7197 |
13.53 |
0.2641 |
1.2641 |
-0.7359 |
|
1476.7227 |
13.57 |
0.2543 |
1.2543 |
-0.7457 |
|
1476.7254 |
13.55 |
0.2455 |
1.2455 |
-0.7545 |
|
1476.7282 |
13.55 |
0.2364 |
1.2364 |
-0.7636 |