PhD Thesis (PDF) - Department of Astronomy - University of Virginia

More documents

Recommendations

Info

Table B.2—Continued RA Dec. d GC G475 Z850 r h Galaxy ACS ID (deg) (deg) (r eff ) (AB) (AB) (pc) Class (1) (2) (3) (4) (5) (6) (7) (8) (9) NGC 4374 116 186.24880 12.87656 1.37 −7.757 ± 0.027 −8.570 ± 0.023 3.10 ± 0.23 1.00 NGC 4374 117 186.25935 12.91296 1.88 −6.564 ± 0.101 −7.089 ± 0.074 3.12 ± 0.71 0.95 NGC 4374 118 186.25298 12.89073 0.91 −7.474 ± 0.025 −8.811 ± 0.034 2.21 ± 0.22 1.00 NGC 4374 120 186.24971 12.87910 1.23 −7.417 ± 0.037 −8.394 ± 0.076 3.88 ± 0.38 1.00 NGC 4374 121 186.25450 12.89513 0.96 −8.452 ± 0.021 −9.735 ± 0.015 1.78 ± 0.11 1.00 NGC 4374 122 186.25900 12.91049 1.72 −8.278 ± 0.025 −9.034 ± 0.046 4.18 ± 0.23 1.00 NGC 4374 123 186.25560 12.89863 1.07 −8.517 ± 0.018 −9.606 ± 0.019 2.47 ± 0.20 1.00 NGC 4374 124 186.24916 12.87617 1.37 −6.416 ± 0.034 −7.253 ± 0.142 1.80 ± 0.42 0.95 NGC 4374 126 186.25238 12.88703 0.91 −9.019 ± 0.020 −10.008 ± 0.023 3.09 ± 0.14 1.00 NGC 4374 129 186.25609 12.89874 1.06 −7.094 ± 0.026 −8.228 ± 0.037 2.71 ± 0.26 1.00 NGC 4374 130 186.25835 12.90614 1.44 −6.501 ± 0.066 −7.646 ± 0.052 3.03 ± 0.31 0.98 NGC 4374 131 186.24941 12.87439 1.43 −8.062 ± 0.019 −9.266 ± 0.026 1.74 ± 0.17 0.98 NGC 4374 132 186.25578 12.89642 0.95 −6.310 ± 0.575 −6.822 ± 0.322 1.34 ± 0.47 0.83 NGC 4374 134 186.25521 12.89227 0.81 −9.310 ± 0.020 −10.228 ± 0.027 10.32 ± 0.16 0.86 NGC 4374 135 186.25890 12.90507 1.36 −7.838 ± 0.040 −8.844 ± 0.048 5.19 ± 0.21 0.99 NGC 4374 136 186.25070 12.87655 1.26 −7.573 ± 0.023 −8.472 ± 0.061 2.93 ± 0.51 1.00 NGC 4374 138 186.25667 12.89688 0.93 −8.783 ± 0.021 −9.706 ± 0.018 2.04 ± 0.14 1.00 NGC 4374 139 186.25573 12.89432 0.85 −7.871 ± 0.018 −8.948 ± 0.339 2.03 ± 0.26 1.00 NGC 4374 140 186.25465 12.88963 0.78 −6.643 ± 0.326 −8.261 ± 0.069 1.80 ± 0.37 0.98 NGC 4374 142 186.25606 12.89417 0.83 −8.013 ± 0.017 −9.325 ± 0.023 2.92 ± 0.16 1.00 NGC 4374 145 186.25321 12.88361 0.89 −8.345 ± 0.026 −9.593 ± 0.014 2.28 ± 0.26 1.00 NGC 4374 147 186.25513 12.89010 0.75 −6.825 ± 0.062 −7.761 ± 0.204 3.73 ± 1.08 0.96 NGC 4374 148 186.25859 12.90155 1.14 −8.769 ± 0.021 −9.641 ± 0.022 2.84 ± 0.16 1.00 NGC 4374 150 186.25891 12.90240 1.18 −7.397 ± 0.030 −8.684 ± 0.028 2.28 ± 0.17 1.00 NGC 4374 153 186.25001 12.87103 1.56 −7.046 ± 0.076 −7.769 ± 0.058 3.73 ± 0.44 0.96 NGC 4374 154 186.25506 12.88847 0.73 −6.544 ± 0.054 −7.751 ± 0.065 2.80 ± 0.43 0.99 NGC 4374 155 186.26057 12.90731 1.48 −7.851 ± 0.028 −9.197 ± 0.028 2.77 ± 0.17 1.00 NGC 4374 156 186.25743 12.89634 0.87 −8.017 ± 0.021 −9.532 ± 0.029 2.32 ± 0.18 1.00 NGC 4374 157 186.26290 12.91530 2.01 −7.521 ± 0.027 −8.890 ± 0.022 2.01 ± 0.17 1.00 NGC 4374 158 186.25966 12.90356 1.24 −8.678 ± 0.017 −9.618 ± 0.016 2.30 ± 0.13 1.00 NGC 4374 163 186.25509 12.88706 0.72 −7.564 ± 0.094 −8.952 ± 0.054 1.80 ± 0.39 1.00 NGC 4374 165 186.25833 12.89814 0.93 −6.301 ± 0.106 −7.511 ± 0.172 3.85 ± 0.91 0.92 NGC 4374 166 186.25104 12.87212 1.45 −8.745 ± 0.021 −9.887 ± 0.019 2.40 ± 0.20 1.00 NGC 4374 167 186.25261 12.87745 1.12 −6.329 ± 0.374 −7.775 ± 0.096 3.49 ± 0.60 0.97 NGC 4374 172 186.26154 12.90726 1.46 −7.789 ± 0.030 −8.811 ± 0.026 2.94 ± 0.17 1.00 NGC 4374 173 186.25575 12.88707 0.68 −7.271 ± 0.043 −8.206 ± 1.109 1.48 ± 0.31 0.95 NGC 4374 174 186.25703 12.89121 0.66 −7.882 ± 0.026 −9.346 ± 0.196 1.59 ± 0.23 0.96 NGC 4374 175 186.25690 12.89031 0.64 −8.277 ± 0.020 −9.076 ± 0.025 2.22 ± 0.21 1.00 NGC 4374 176 186.25607 12.88750 0.66 −6.595 ± 0.181 −7.591 ± 0.054 1.79 ± 0.40 0.96 NGC 4374 177 186.25639 12.88847 0.64 −6.447 ± 0.058 −7.583 ± 0.076 2.34 ± 0.39 0.99 NGC 4374 179 186.25292 12.87549 1.19 −7.209 ± 0.039 −8.171 ± 0.062 4.29 ± 0.33 0.97 NGC 4374 181 186.25780 12.89173 0.63 −7.656 ± 0.027 −8.987 ± 0.031 1.69 ± 0.22 0.98 NGC 4374 182 186.24958 12.86292 2.03 −7.783 ± 0.025 −8.903 ± 0.039 3.43 ± 0.26 1.00 NGC 4374 183 186.25885 12.89512 0.74 −8.526 ± 0.026 −9.529 ± 0.018 2.12 ± 0.13 1.00 NGC 4374 187 186.26088 12.90178 1.09 −9.098 ± 0.024 −10.626 ± 0.021 2.47 ± 0.27 1.00 NGC 4374 188 186.26282 12.90865 1.54 −6.849 ± 0.087 −7.986 ± 0.118 5.63 ± 0.63 0.82 NGC 4374 189 186.24966 12.86274 2.04 −7.485 ± 0.030 −8.527 ± 0.040 3.33 ± 0.26 1.00 NGC 4374 190 186.26323 12.90901 1.56 −8.562 ± 0.027 −9.575 ± 0.043 5.63 ± 0.17 0.99 NGC 4374 192 186.26135 12.90219 1.11 −6.727 ± 0.040 −8.162 ± 0.055 1.77 ± 0.33 0.98 NGC 4374 193 186.26103 12.90096 1.04 −6.776 ± 0.116 −7.570 ± 0.538 3.60 ± 1.12 0.95 NGC 4374 194 186.25009 12.86284 2.01 −7.214 ± 0.029 −8.189 ± 0.054 2.56 ± 0.26 1.00 NGC 4374 197 186.25227 12.86989 1.52 −6.536 ± 0.033 −7.896 ± 0.097 3.75 ± 0.36 0.97 NGC 4374 199 186.25230 12.86960 1.53 −8.709 ± 0.020 −9.908 ± 0.023 3.77 ± 0.15 1.00 NGC 4374 200 186.26116 12.89964 0.94 −8.526 ± 0.015 −9.520 ± 0.020 2.50 ± 0.09 1.00 NGC 4374 201 186.26311 12.90644 1.38 −5.511 ± 0.271 −6.493 ± 0.431 2.06 ± 1.54 0.93 NGC 4374 202 186.25191 12.86724 1.69 −8.004 ± 0.029 −8.855 ± 0.029 2.88 ± 0.23 1.00 NGC 4374 203 186.26393 12.90906 1.56 −6.883 ± 0.057 −7.707 ± 0.047 3.22 ± 0.35 0.98 NGC 4374 204 186.25083 12.86320 1.97 −8.266 ± 0.016 −9.142 ± 0.025 3.31 ± 0.17 1.00 NGC 4374 205 186.26123 12.89953 0.93 −6.669 ± 0.036 −7.658 ± 0.049 2.64 ± 0.22 0.99 NGC 4374 206 186.25742 12.88595 0.57 −7.630 ± 0.032 −9.017 ± 0.065 2.69 ± 0.36 1.00 NGC 4374 207 186.25994 12.89455 0.66 −6.426 ± 0.117 −7.431 ± 0.182 3.67 ± 1.44 0.93 NGC 4374 208 186.25725 12.88449 0.60 −8.184 ± 0.079 −9.457 ± 0.021 1.43 ± 0.20 0.94 Continued on Next Page. . . 312
Table B.2—Continued RA Dec. d GC G475 Z850 r h Galaxy ACS ID (deg) (deg) (r eff ) (AB) (AB) (pc) Class (1) (2) (3) (4) (5) (6) (7) (8) (9) NGC 4374 209 186.25836 12.88820 0.51 −7.900 ± 0.026 −8.898 ± 0.046 3.21 ± 0.20 1.00 NGC 4374 210 186.26601 12.91482 1.97 −6.687 ± 0.035 −7.806 ± 0.045 2.33 ± 0.33 0.99 NGC 4374 211 186.25620 12.87992 0.82 −6.576 ± 0.223 −7.774 ± 0.170 6.39 ± 2.28 0.61 NGC 4374 212 186.26073 12.89554 0.69 −6.300 ± 0.113 −7.979 ± 0.133 3.90 ± 0.84 0.97 NGC 4374 213 186.25769 12.88489 0.57 −7.834 ± 0.021 −8.772 ± 0.053 2.59 ± 0.26 1.00 NGC 4374 217 186.25791 12.88421 0.57 −8.030 ± 0.152 −9.354 ± 0.250 1.47 ± 0.30 0.95 NGC 4374 218 186.25899 12.88788 0.46 −7.253 ± 0.090 −8.409 ± 0.095 6.87 ± 0.59 0.74 NGC 4374 219 186.25975 12.89045 0.47 −8.184 ± 0.029 −9.612 ± 0.024 1.85 ± 0.20 1.00 NGC 4374 222 186.25893 12.88705 0.46 −6.161 ± 1.161 −7.494 ± 0.164 1.82 ± 0.51 0.96 NGC 4374 223 186.26421 12.90509 1.28 −7.308 ± 0.053 −8.099 ± 0.072 2.77 ± 0.30 0.99 NGC 4374 224 186.25702 12.87962 0.79 −8.199 ± 0.052 −9.359 ± 0.059 1.40 ± 0.30 0.94 NGC 4374 225 186.25968 12.88881 0.43 −8.665 ± 0.030 −9.713 ± 0.030 2.42 ± 0.19 1.00 NGC 4374 226 186.25894 12.88607 0.46 −7.969 ± 0.020 −8.882 ± 0.052 2.98 ± 0.22 1.00 NGC 4374 227 186.25861 12.88465 0.51 −7.903 ± 0.054 −9.003 ± 0.093 5.53 ± 0.49 0.98 NGC 4374 228 186.25824 12.88335 0.57 −8.046 ± 0.021 −9.017 ± 0.032 1.89 ± 0.24 1.00 NGC 4374 229 186.25838 12.88336 0.56 −8.845 ± 0.020 −10.066 ± 0.021 2.17 ± 0.15 1.00 NGC 4374 230 186.26070 12.89203 0.49 −7.616 ± 0.045 −9.296 ± 0.034 1.90 ± 0.32 1.00 NGC 4374 231 186.26003 12.88936 0.42 −8.350 ± 0.022 −9.787 ± 0.019 2.06 ± 0.24 1.00 NGC 4374 232 186.25593 12.87469 1.10 −6.170 ± 0.078 −7.318 ± 0.372 1.28 ± 0.41 0.85 NGC 4374 233 186.26126 12.89311 0.53 −9.268 ± 0.017 −10.202 ± 0.019 2.70 ± 0.21 1.00 NGC 4374 234 186.26071 12.89083 0.43 −8.480 ± 0.027 −9.437 ± 0.031 2.94 ± 0.29 1.00 NGC 4374 235 186.26244 12.89696 0.74 −9.841 ± 0.012 −10.922 ± 0.011 2.89 ± 0.13 1.00 NGC 4374 236 186.26227 12.89605 0.68 −8.676 ± 0.023 −9.882 ± 0.020 2.35 ± 0.16 1.00 NGC 4374 237 186.25822 12.88189 0.62 −5.326 ± 0.691 −7.088 ± 0.157 3.03 ± 1.77 0.95 NGC 4374 238 186.26462 12.90317 1.14 −6.581 ± 0.199 −7.498 ± 0.097 2.85 ± 0.46 0.98 NGC 4374 239 186.26520 12.90510 1.28 −6.490 ± 0.052 −7.693 ± 0.039 2.29 ± 0.34 0.99 NGC 4374 240 186.26566 12.90658 1.38 −6.339 ± 0.060 −7.947 ± 0.067 2.61 ± 0.37 0.99 NGC 4374 241 186.26253 12.89558 0.64 −9.132 ± 0.020 −9.968 ± 0.044 3.90 ± 0.21 1.00 NGC 4374 242 186.25464 12.86735 1.58 −9.121 ± 0.040 −10.067 ± 0.052 6.74 ± 0.35 1.00 NGC 4374 243 186.25600 12.87168 1.27 −7.451 ± 0.034 −8.620 ± 0.034 3.29 ± 0.31 1.00 NGC 4374 244 186.25972 12.88484 0.43 −10.076 ± 0.013 −11.557 ± 0.021 2.55 ± 0.09 1.00 NGC 4374 245 186.25386 12.86401 1.82 −7.429 ± 0.035 −8.530 ± 0.044 3.12 ± 0.23 1.00 NGC 4374 246 186.26437 12.90031 0.94 −6.156 ± 0.095 −7.854 ± 0.139 5.68 ± 1.07 0.77 NGC 4374 247 186.25733 12.87515 1.01 −9.816 ± 0.023 −10.688 ± 0.026 3.93 ± 0.13 1.00 NGC 4374 250 186.26653 12.90691 1.41 −7.443 ± 0.019 −8.760 ± 0.022 2.39 ± 0.17 1.00 NGC 4374 252 186.26667 12.90728 1.43 −5.498 ± 0.110 −6.688 ± 0.300 4.74 ± 3.22 0.53 NGC 4374 254 186.25528 12.86694 1.59 −6.302 ± 0.118 −7.530 ± 0.047 2.53 ± 0.37 0.99 NGC 4374 255 186.26876 12.91387 1.91 −5.386 ± 0.441 −6.812 ± 0.069 2.09 ± 0.71 0.95 NGC 4374 257 186.25607 12.86938 1.41 −5.948 ± 0.057 −6.577 ± 0.763 1.43 ± 0.49 0.84 NGC 4374 259 186.26901 12.91431 1.94 −6.085 ± 0.919 −7.800 ± 0.151 4.04 ± 40.80 0.94 NGC 4374 260 186.25963 12.88130 0.58 −7.694 ± 0.027 −8.548 ± 0.048 2.55 ± 0.19 1.00 NGC 4374 261 186.26225 12.89029 0.33 −8.149 ± 0.021 −9.122 ± 0.281 2.33 ± 0.24 1.00 NGC 4374 264 186.26684 12.90554 1.31 −6.694 ± 0.041 −7.638 ± 0.099 1.98 ± 0.53 0.98 NGC 4374 266 186.26067 12.88359 0.42 −9.400 ± 0.020 −10.364 ± 0.016 1.87 ± 0.18 1.00 NGC 4374 267 186.26342 12.89318 0.46 −8.692 ± 0.015 −9.712 ± 0.026 2.79 ± 0.21 1.00 NGC 4374 269 186.25614 12.86764 1.52 −6.656 ± 0.064 −7.614 ± 0.046 2.98 ± 0.32 0.98 NGC 4374 270 186.26137 12.88514 0.32 −8.923 ± 0.026 −10.007 ± 0.023 2.81 ± 0.19 1.00 NGC 4374 271 186.26920 12.91249 1.82 −7.027 ± 0.046 −8.095 ± 0.047 3.05 ± 0.32 0.99 NGC 4374 272 186.26415 12.89427 0.52 −8.573 ± 0.018 −9.580 ± 0.028 2.50 ± 0.20 1.00 NGC 4374 275 186.26762 12.90526 1.30 −6.265 ± 0.072 −7.531 ± 0.061 2.19 ± 0.49 0.98 NGC 4374 276 186.25669 12.86679 1.55 −7.149 ± 0.025 −8.119 ± 0.317 1.50 ± 0.32 0.95 NGC 4374 277 186.26810 12.90629 1.37 −9.101 ± 0.022 −10.074 ± 0.012 2.46 ± 0.12 1.00 NGC 4374 278 186.26987 12.91257 1.83 −7.046 ± 0.045 −8.006 ± 0.079 3.69 ± 0.46 0.98 NGC 4374 279 186.25568 12.86262 1.85 −5.296 ± 0.583 −6.217 ± 0.519 1.84 ± 1.31 0.91 NGC 4374 280 186.26907 12.90906 1.58 −5.787 ± 0.064 −7.163 ± 0.247 2.39 ± 0.60 0.98 NGC 4374 281 186.26357 12.88994 0.25 −7.750 ± 0.029 −8.742 ± 0.042 2.22 ± 0.22 1.00 NGC 4374 282 186.26028 12.87795 0.74 −7.144 ± 0.050 −8.148 ± 0.041 2.12 ± 0.29 0.99 NGC 4374 283 186.26578 12.89705 0.71 −8.108 ± 0.029 −8.822 ± 0.027 3.25 ± 0.16 1.00 NGC 4374 284 186.26378 12.88955 0.22 −9.089 ± 0.064 −9.878 ± 0.030 2.88 ± 0.26 1.00 NGC 4374 285 186.25981 12.87571 0.89 −8.131 ± 0.056 −9.494 ± 0.022 2.59 ± 0.31 1.00 NGC 4374 286 186.26372 12.88936 0.21 −8.655 ± 0.022 −9.999 ± 0.032 2.68 ± 0.17 1.00 NGC 4374 288 186.26132 12.88044 0.55 −6.165 ± 0.671 −7.117 ± 0.151 1.64 ± 0.62 0.92 Continued on Next Page. . . 313
Page 1 and 2:
LOW-MASS X-RAY BINARIES, DIFFUSE GA
Page 3 and 4:
smaller GCs are more likely to cont
Page 5 and 6:
GO2-3099X, GO3-4099X, AR3-4005X, GO
Page 7 and 8:
her room (my apologies to her offic
Page 9 and 10:
US Court expert from India), for al
Page 11 and 12:
Table of contents Abstract ii Ackno
Page 13 and 14:
5.2.1 Chandra X-ray Observatory . .
Page 15 and 16:
List of Figures 1.1 Hubble Tuning F
Page 17 and 18:
List of Tables 1.1 Galactic Low-Mas
Page 19 and 20:
Chapter 1 General Introduction 1.1
Page 21 and 22:
Fig. 1.1.— Hubble Tuning Fork, co
Page 23 and 24:
2000). In most HMXBs, the accreted
Page 25 and 26:
not get a complete picture of the L
Page 27 and 28:
this, the result of dynamical inter
Page 29 and 30:
is the Advanced CCD Imaging Spectro
Page 31 and 32:
Chapter 2 Chandra Observations of L
Page 33 and 34:
keV (Sarazin et al. 2000, 2001). Wi
Page 35 and 36:
agreed with positions from the USNO
Page 37 and 38:
24:00 22:00 7:20:00 18:00 16:00 18:
Page 39 and 40:
Table 2.1. Discrete X-ray Sources i
Page 41 and 42:
Table 2.1—Continued Source d Coun
Page 43 and 44:
Page 45 and 46:
Table 2.2—Continued Source d Coun
Page 47 and 48:
optical/IR positions of R.A. = 12 h
Page 49 and 50:
log N(>L) 2.0 1.5 1.0 0.5 0.0 NGC 4
Page 51 and 52:
luminosity function for luminositie
Page 53 and 54:
H31 1.0 0.5 0.0 -0.5 -1.0 NGC 4365
Page 55 and 56:
2.4.5 Variability We searched for v
Page 57 and 58:
Number 10 8 6 4 2 NGC 4365 Optical
Page 59 and 60:
LMXBs has an effective radius of 12
Page 61 and 62:
component (“MEKAL”) was used fo
Page 63 and 64:
Table 2.4. X-ray Spectral Fits of N
Page 65 and 66:
Fig. 2.9.— Top panels: Cumulative
Page 67 and 68:
we extended the spectrum down to 0.
Page 69 and 70:
We also examined whether the unreso
Page 71 and 72:
esolved sources in the galaxy. This
Page 73 and 74:
temperature ∼0.3 keV. Matsumoto e
Page 75 and 76:
log I X (counts/sec/arcmin 2 ) -1.0
Page 77 and 78:
∼45% of the counts are resolved i
Page 79 and 80:
Chapter 3 Chandra Observations of D
Page 81 and 82:
noninteracting members (de Vaucoule
Page 83 and 84:
used for spectroscopic analysis. We
Page 85 and 86:
02:00.0 03:00.0 04:00.0 05:00.0 06:
Page 87 and 88:
Page 89 and 90:
Table 3.1—Continued d a Count Rat
Page 91 and 92:
We also attempted detections in mul
Page 93 and 94:
sociated with extended X-ray or opt
Page 95 and 96:
Fig. 3.3.— Histogram of the obser
Page 97 and 98:
chip. The number of ULX candidates
Page 99 and 100:
these luminosities among previously
Page 101 and 102:
to 2-6 keV. Since the 6-10 keV rang
Page 103 and 104:
absorption and varying power-law in
Page 105 and 106:
counts occur within ∼ 4 ks. Sourc
Page 107 and 108:
log I X (counts/sec/arcmin 2 ) 0.5
Page 109 and 110:
tion), and βouter = 0.36 +0.01 −
Page 111 and 112:
the east and northeast of NGC 1600.
Page 113 and 114:
group, we assumed that they were at
Page 115 and 116:
the group gas than we calculate fro
Page 117 and 118:
04:55 -5:05:00 05 -5:05:10 15 -5:05
Page 119 and 120:
for the spectrum: “Field” impli
Page 121 and 122:
90% confidence level errors. Bracke
Page 123 and 124:
we adopted the power-law model as o
Page 125 and 126:
sources could be a non-trivial sour
Page 127 and 128:
jection to include the emission fro
Page 129 and 130:
Fig. 3.13.— Estimated gas and gra
Page 131 and 132:
ackground source population cannot
Page 133 and 134:
NGC 1600 that has a small spatial s
Page 135 and 136:
(HMXBs). LMC X-4, an HMXB pulsar, h
Page 137 and 138:
searched for the shortest time tn o
Page 139 and 140:
with NGC 4697. Columns (1)-(4) list
Page 141 and 142:
duration, ∆tflat, beginning at a
Page 143 and 144:
the uncertainties quoted do not inc
Page 145 and 146:
to persistent rate for short flares
Page 147 and 148:
Chapter 5 Multi-Epoch Chandra X-ray
Page 149 and 150:
the field, these different populati
Page 151 and 152:
luminous (MB < −20) elliptical (E
Page 153 and 154:
Although Chandra is known to encoun
Page 155 and 156:
42:00.0 44:00.0 46:00.0 48:00.0 -5:
Page 157 and 158:
Fig. 5.3.— Adaptively smoothed Ch
Page 159 and 160:
1 × 10 −5 count s −1 arcsec
Page 161 and 162:
Table 5.1—Continued Source R.A. D
Page 163 and 164:
Page 165 and 166:
Page 167 and 168:
source list against which to regist
Page 169 and 170:
ate from Observation 0784 alone (Pa
Page 171 and 172:
Table 5.2. : Optical Properties of
Page 173 and 174:
actually be an AGN. Sources 79, 80,
Page 175 and 176:
two potential GC counterparts. We l
Page 177 and 178:
Table 5.3—Continued X-ray Source
Page 179 and 180:
Fig. 5.6.— Color (G475−Z850) -
Page 181 and 182:
mass segregation of GCs with the sa
Page 183 and 184:
Table 5.4. Fits to the Expected Num
Page 185 and 186:
dependence are allowed to vary. Var
Page 187 and 188:
NGC 4697 to convert the observed so
Page 189 and 190:
Table 5.6—Continued Source LA LB
Page 191 and 192:
Table 5.6—Continued Source LA LB
Page 193 and 194:
Table 5.7. Combined Luminosities &
Page 195 and 196:
Table 5.7—Continued Source Not De
Page 197 and 198:
Fig. 5.8.— Cumulative luminosity
Page 199 and 200:
LF, there are enough datapoints tha
Page 201 and 202:
Fig. 5.10.— Cumulative luminosity
Page 203 and 204:
Fig. 5.11.— Merged luminosities (
Page 205 and 206:
Fig. 5.12.— X-ray color-color dia
Page 207 and 208:
5.9 Spectral Analysis We performed
Page 209 and 210:
some data loss, it allows for direc
Page 211 and 212:
for 2 dof and the f-test indicates
Page 213 and 214:
ple to LMXBs interior to that semi-
Page 215 and 216:
est-fit (χ 2 = 56.4 for 65 dof) by
Page 217 and 218:
5.10.1 Intraobservation Variability
Page 219 and 220:
Fig. 5.14.— Binned lightcurve usi
Page 221 and 222:
Table 5.10. Possible Flaring Source
Page 223 and 224:
Fig. 5.16.— Cumulative lightcurve
Page 225 and 226:
pairs of observations. In Figure 5.
Page 227 and 228:
Table 5.11—Continued Source PL,AB
Page 229 and 230:
Fig. 5.17.— Percentage of Analysi
Page 231 and 232:
dofs and the number of combinations
Page 233 and 234:
Table 5.12—Continued Source Obs.S
Page 235 and 236:
of states as transient candidates.
Page 237 and 238:
Long-Term Hardness Ratio Variabilit
Page 239 and 240:
In the final observation, there wer
Page 241 and 242:
limits). The 0.3-10 keV X-ray lumin
Page 243 and 244:
atio is expected only from the most
Page 245 and 246:
eak (Kim et al. 2006a). We find mar
Page 247 and 248:
LMXBs in Galactic GCs (Heinke et al
Page 249 and 250:
in the field of the Milky Way and a
Page 251 and 252:
6.2 Sample 6.2.1 Galaxy Sample Tabl
Page 253 and 254:
Table 6.2. Properties of Chandra Ob
Page 255 and 256:
identification of point sources, AC
Page 257 and 258:
the QE degradation in the ACIS dete
Page 259 and 260:
Table 6.3—Continued Galaxy NX LX,
Page 261 and 262:
The positions of the GCs were used
Page 263 and 264:
Fig. 6.2.— Scatter plot of GC gal
Page 265 and 266:
Fig. 6.3.— Scatter plot of estima
Page 267 and 268:
Fig. 6.5.— Scatter plot of estima
Page 269 and 270:
isophote from the galaxy optical su
Page 271 and 272:
6.3.1 Luminosity and Mass Prior obs
Page 273 and 274:
compare their χ 2 fits to test whi
Page 275 and 276:
GCs without LMXBs; however, there a
Page 277 and 278:
following dependence on GC properti
Page 279 and 280: of this probability with individual
Page 281 and 282: Fig. 6.9.— Identical to Figure 6.
Page 283 and 284: We used the indices from our best-f
Page 285 and 286: (20.3 for half-mass radius, both wi
Page 287 and 288: most are steeper than Z ∼0.4 . Ei
Page 289 and 290: Fig. 6.11.— (Left:) Two-dimension
Page 291 and 292: differently by the properties of th
Page 293 and 294: dependent IMF (Grindlay 1987), or e
Page 295 and 296: a 1.4M⊙ neutron star (NS). They s
Page 297 and 298: equivalent to a dependence on the b
Page 299 and 300: variability timescale, but it is no
Page 301 and 302: 7.2.1 X-ray Properties of the GC-LM
Page 303 and 304: of the metallicity dependence. As i
Page 305 and 306: Appendix A Encounter Rate Parameter
Page 307 and 308: Fig. A.1.— Dimensionless quantity
Page 309 and 310: and four; these positions do not in
Page 311 and 312: Table B.1—Continued RA Dec. d GC
Page 315 and 316: Table B.2. Optical Properties of Gl
Page 329: Table B.2—Continued RA Dec. d GC
Page 381 and 382:
Table B.2—Continued RA Dec. d GC
Page 383 and 384:
Page 385 and 386:
Page 387 and 388:
Page 389 and 390:
Page 391 and 392:
Page 393 and 394:
Page 395 and 396:
Page 397 and 398:
Page 399 and 400:
Page 401 and 402:
Page 403 and 404:
Page 405 and 406:
Page 407 and 408:
Page 409 and 410:
Page 411 and 412:
Page 413 and 414:
Page 415 and 416:
Page 417 and 418:
Page 419 and 420:
Page 421 and 422:
investigations into improving the h
Page 423 and 424:
C.4 Sivakoff Signature Soy Sauce Sk
Page 425 and 426:
Blanton, E. L., Sarazin, C. L., & I
Page 427 and 428:
Frogel, J. A., Persson, S. E., Matt
Page 429 and 430:
Johnston, H. M. & Verbunt, F. 1996,
Page 431 and 432:
Makishima, K. et al. 2000, ApJ, 535
Page 433 and 434:
Porter, A. C. 1993, PASP, 105, 1250
Page 435:
Verner, D. A., Ferland, G. J., Kori
show all

PhD Thesis (PDF) - Department of Astronomy - University of Virginia

You also want an ePaper? Increase the reach of your titles

Delete template?

Save as template?