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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 662 186.28939 12.87370 1.89 −9.371 ± 0.007 −10.254 ± 0.014 3.39 ± 0.07 1.00 NGC 4374 663 186.28460 12.85511 2.61 −6.859 ± 0.075 −7.429 ± 0.082 4.34 ± 0.31 0.85 NGC 4374 665 186.29480 12.88955 2.02 −8.662 ± 0.026 −9.548 ± 0.024 2.49 ± 0.18 1.00 NGC 4374 670 186.29577 12.89099 2.10 −9.002 ± 0.021 −10.321 ± 0.018 2.97 ± 0.17 1.00 NGC 4374 671 186.29256 12.87984 1.92 −8.661 ± 0.012 −9.665 ± 0.015 2.26 ± 0.10 1.00 NGC 4374 672 186.29523 12.88893 2.04 −8.331 ± 0.025 −9.522 ± 0.027 2.82 ± 0.18 1.00 NGC 4374 673 186.29026 12.87155 2.02 −6.676 ± 0.073 −7.602 ± 0.104 3.91 ± 0.55 0.93 NGC 4374 674 186.28713 12.86035 2.40 −7.010 ± 0.026 −8.211 ± 0.063 3.00 ± 0.35 0.99 NGC 4374 678 186.29575 12.88841 2.08 −8.943 ± 0.065 −10.234 ± 0.065 7.73 ± 0.50 1.00 NGC 4374 680 186.29251 12.87716 1.98 −7.561 ± 0.052 −8.739 ± 0.041 3.26 ± 0.23 1.00 NGC 4374 681 186.29811 12.89664 2.34 −6.195 ± 0.135 −6.833 ± 0.121 3.12 ± 0.75 0.93 NGC 4374 682 186.29005 12.86762 2.17 −7.633 ± 0.028 −8.546 ± 0.036 2.53 ± 0.26 1.00 NGC 4374 683 186.29872 12.89750 2.40 −5.437 ± 0.151 −6.859 ± 0.061 3.47 ± 0.67 0.89 NGC 4374 684 186.28937 12.86457 2.28 −9.001 ± 0.027 −10.069 ± 0.020 2.83 ± 0.26 1.00 NGC 4374 686 186.29351 12.87898 2.00 −6.597 ± 0.049 −7.697 ± 0.096 4.70 ± 0.46 0.87 NGC 4374 687 186.28926 12.86415 2.29 −7.086 ± 0.032 −8.354 ± 0.033 2.96 ± 0.30 0.99 NGC 4374 690 186.29236 12.87413 2.06 −8.182 ± 0.019 −9.587 ± 0.019 2.83 ± 0.12 1.00 NGC 4374 693 186.29000 12.86541 2.27 −6.846 ± 0.048 −8.116 ± 0.081 4.17 ± 0.41 0.97 NGC 4374 699 186.29937 12.89505 2.39 −6.271 ± 0.063 −7.429 ± 0.080 2.34 ± 0.38 0.99 NGC 4374 700 186.29694 12.88636 2.16 −7.889 ± 0.019 −9.273 ± 0.020 2.09 ± 0.12 1.00 NGC 4374 702 186.28924 12.85819 2.61 −9.139 ± 0.015 −10.006 ± 0.012 3.11 ± 0.08 1.00 NGC 4374 703 186.29259 12.86937 2.24 −6.941 ± 0.076 −7.624 ± 0.064 2.61 ± 0.36 0.99 NGC 4374 705 186.30008 12.89480 2.44 −8.089 ± 0.020 −9.018 ± 0.023 2.27 ± 0.17 1.00 NGC 4374 708 186.30207 12.90080 2.69 −7.711 ± 0.032 −8.675 ± 0.023 2.93 ± 0.22 1.00 NGC 4374 709 186.29091 12.86165 2.50 −7.417 ± 0.028 −8.629 ± 0.027 2.34 ± 0.22 1.00 NGC 4374 711 186.29467 12.87406 2.20 −7.180 ± 0.138 −8.786 ± 0.092 5.92 ± 0.88 0.93 NGC 4374 712 186.30395 12.90605 2.96 −9.432 ± 0.022 −10.421 ± 0.022 3.20 ± 0.14 1.00 NGC 4374 716 186.29439 12.87168 2.26 −8.684 ± 0.023 −9.685 ± 0.023 3.30 ± 0.18 1.00 NGC 4374 717 186.29331 12.86750 2.35 −6.232 ± 0.107 −7.333 ± 0.131 3.10 ± 0.88 0.96 NGC 4374 722 186.29513 12.87303 2.26 −6.506 ± 1.015 −8.248 ± 0.267 1.27 ± 0.35 0.90 NGC 4374 723 186.29337 12.86623 2.41 −6.850 ± 0.062 −7.880 ± 0.086 4.22 ± 0.43 0.94 NGC 4374 729 186.29716 12.87792 2.27 −7.528 ± 0.030 −8.986 ± 0.016 2.60 ± 0.17 1.00 NGC 4374 731 186.29600 12.87267 2.33 −7.380 ± 0.037 −8.226 ± 0.030 2.83 ± 0.24 0.99 NGC 4374 732 186.29661 12.87438 2.31 −6.949 ± 0.056 −8.293 ± 0.044 3.21 ± 0.27 0.99 NGC 4374 735 186.29624 12.87224 2.35 −9.106 ± 0.030 −10.383 ± 0.018 2.95 ± 0.17 1.00 NGC 4374 738 186.29950 12.88328 2.35 −7.533 ± 0.029 −8.293 ± 0.030 2.62 ± 0.20 1.00 NGC 4374 742 186.30232 12.89234 2.56 −7.610 ± 0.036 −8.657 ± 0.031 3.70 ± 0.25 1.00 NGC 4374 743 186.30498 12.90161 2.90 −6.065 ± 0.086 −6.727 ± 0.076 3.33 ± 0.48 0.90 NGC 4374 744 186.29115 12.85388 2.93 −5.224 ± 0.276 −6.701 ± 0.236 3.68 ± 1.40 0.85 NGC 4374 746 186.29975 12.88283 2.37 −6.050 ± 0.105 −7.723 ± 0.293 6.01 ± 3.63 0.67 NGC 4374 749 186.30388 12.89600 2.71 −7.613 ± 0.025 −8.596 ± 0.035 4.14 ± 0.22 1.00 NGC 4374 756 186.30460 12.89570 2.76 −7.347 ± 0.034 −8.381 ± 0.045 4.54 ± 0.31 1.00 NGC 4374 757 186.30033 12.88078 2.43 −7.679 ± 0.037 −9.052 ± 0.021 2.66 ± 0.22 1.00 NGC 4374 760 186.30600 12.89909 2.91 −6.982 ± 0.047 −7.834 ± 0.076 3.59 ± 0.46 0.97 NGC 4374 763 186.30638 12.89871 2.93 −7.399 ± 0.056 −8.530 ± 0.038 4.30 ± 0.28 1.00 NGC 4382 1 186.32349 18.17222 2.09 −7.019 ± 0.057 −7.769 ± 0.074 2.66 ± 0.36 0.95 NGC 4382 5 186.32552 18.18377 1.62 −5.328 ± 0.131 −6.231 ± 0.703 2.91 ± 0.71 0.80 NGC 4382 6 186.32346 18.16755 2.29 −5.236 ± 0.182 −6.829 ± 0.151 4.03 ± 1.17 0.59 NGC 4382 7 186.32457 18.17407 1.96 −7.725 ± 0.033 −8.607 ± 0.040 3.94 ± 0.22 1.00 NGC 4382 10 186.32678 18.18902 1.48 −5.807 ± 0.083 −7.212 ± 0.074 3.24 ± 0.32 0.84 NGC 4382 11 186.32636 18.18449 1.56 −6.827 ± 0.049 −7.951 ± 0.036 2.71 ± 0.26 0.97 NGC 4382 12 186.32697 18.18784 1.47 −6.762 ± 0.036 −7.891 ± 0.058 3.04 ± 0.24 0.95 NGC 4382 17 186.32550 18.17319 1.95 −5.931 ± 0.106 −7.207 ± 0.172 4.47 ± 0.93 0.54 NGC 4382 19 186.32725 18.18584 1.48 −8.245 ± 0.080 −9.149 ± 0.074 3.22 ± 0.39 1.00 NGC 4382 20 186.32805 18.19185 1.39 −6.362 ± 0.073 −7.569 ± 0.096 4.09 ± 0.51 0.80 NGC 4382 24 186.32683 18.18070 1.62 −7.384 ± 0.063 −8.042 ± 0.100 5.79 ± 0.59 0.62 NGC 4382 28 186.32555 18.16897 2.13 −7.923 ± 0.030 −8.791 ± 0.027 3.26 ± 0.14 1.00 NGC 4382 30 186.32598 18.16923 2.09 −6.444 ± 0.081 −7.379 ± 0.042 3.13 ± 0.38 0.89 NGC 4382 31 186.33126 18.20877 1.67 −8.954 ± 0.014 −10.187 ± 0.015 3.13 ± 0.12 1.00 NGC 4382 33 186.32938 18.19357 1.32 −7.800 ± 0.029 −8.978 ± 0.026 1.83 ± 0.20 1.00 NGC 4382 34 186.32642 18.17048 2.02 −7.790 ± 0.031 −8.722 ± 0.023 2.74 ± 0.21 1.00 Continued on Next Page. . . 318
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 4382 35 186.32901 18.19044 1.33 −7.412 ± 0.046 −9.057 ± 0.064 4.72 ± 0.47 1.00 NGC 4382 44 186.32986 18.19240 1.28 −6.999 ± 0.053 −8.136 ± 0.067 2.76 ± 0.40 0.97 NGC 4382 49 186.33157 18.20371 1.43 −6.355 ± 0.071 −7.774 ± 0.058 5.44 ± 0.31 0.55 NGC 4382 56 186.32767 18.17000 1.98 −8.090 ± 0.070 −9.104 ± 0.101 2.65 ± 0.45 1.00 NGC 4382 57 186.33335 18.21380 1.83 −9.044 ± 0.013 −10.462 ± 0.016 3.21 ± 0.08 1.00 NGC 4382 63 186.32950 18.18295 1.41 −8.291 ± 0.027 −9.122 ± 0.033 2.87 ± 0.17 1.00 NGC 4382 66 186.33179 18.19938 1.28 −8.290 ± 0.036 −9.221 ± 0.082 8.28 ± 0.58 0.52 NGC 4382 70 186.33111 18.19347 1.21 −5.007 ± 0.487 −6.215 ± 0.443 3.55 ± 1.49 0.76 NGC 4382 72 186.33208 18.19994 1.28 −9.379 ± 0.027 −10.225 ± 0.017 3.73 ± 0.12 1.00 NGC 4382 77 186.33045 18.18627 1.28 −8.687 ± 0.017 −9.749 ± 0.020 2.60 ± 0.16 1.00 NGC 4382 78 186.33208 18.19753 1.21 −5.599 ± 0.199 −6.388 ± 0.128 3.74 ± 1.43 0.69 NGC 4382 84 186.33416 18.21128 1.67 −5.718 ± 0.074 −6.451 ± 0.606 2.24 ± 0.47 0.76 NGC 4382 85 186.33357 18.20601 1.43 −8.129 ± 0.051 −8.992 ± 0.052 5.08 ± 0.29 0.98 NGC 4382 87 186.33350 18.20501 1.39 −5.570 ± 0.121 −7.016 ± 0.120 3.77 ± 0.63 0.69 NGC 4382 90 186.33058 18.18057 1.41 −7.518 ± 0.037 −9.028 ± 0.027 3.06 ± 0.18 1.00 NGC 4382 93 186.33152 18.18719 1.20 −6.422 ± 0.093 −7.529 ± 0.095 3.96 ± 0.49 0.80 NGC 4382 97 186.33325 18.19896 1.18 −5.714 ± 0.470 −7.091 ± 0.132 3.58 ± 1.47 0.75 NGC 4382 98 186.33502 18.21245 1.70 −7.648 ± 0.024 −8.909 ± 0.034 2.83 ± 0.16 1.00 NGC 4382 100 186.33017 18.17461 1.66 −5.832 ± 0.122 −7.492 ± 0.144 4.66 ± 0.83 0.62 NGC 4382 101 186.33228 18.19088 1.13 −7.137 ± 0.043 −8.372 ± 0.045 3.20 ± 0.23 1.00 NGC 4382 102 186.33331 18.19858 1.17 −7.108 ± 0.060 −8.062 ± 0.029 2.50 ± 0.26 0.97 NGC 4382 103 186.33185 18.18706 1.18 −6.830 ± 0.050 −8.203 ± 0.030 1.41 ± 0.31 0.51 NGC 4382 104 186.33327 18.19817 1.16 −5.105 ± 0.106 −6.581 ± 0.123 3.05 ± 0.59 0.79 NGC 4382 105 186.33220 18.18834 1.14 −6.940 ± 0.038 −8.204 ± 0.048 1.44 ± 0.22 0.54 NGC 4382 107 186.33331 18.19592 1.11 −9.772 ± 0.020 −10.918 ± 0.011 2.38 ± 0.10 1.00 NGC 4382 108 186.32957 18.16710 2.04 −6.882 ± 0.062 −8.048 ± 0.059 3.60 ± 0.32 0.94 NGC 4382 111 186.33594 18.21313 1.71 −5.136 ± 0.163 −6.361 ± 0.275 3.58 ± 1.94 0.73 NGC 4382 113 186.33579 18.21132 1.61 −8.165 ± 0.034 −9.075 ± 0.042 4.70 ± 0.19 1.00 NGC 4382 115 186.33532 18.20830 1.47 −6.988 ± 0.036 −7.949 ± 0.035 2.13 ± 0.29 0.95 NGC 4382 116 186.33376 18.19469 1.06 −5.218 ± 0.727 −6.361 ± 0.162 2.43 ± 0.64 0.78 NGC 4382 120 186.33087 18.16964 1.86 −7.445 ± 0.056 −8.648 ± 0.043 4.01 ± 0.23 1.00 NGC 4382 125 186.33153 18.17278 1.68 −7.682 ± 0.027 −8.854 ± 0.348 1.79 ± 0.23 1.00 NGC 4382 126 186.33613 18.20866 1.46 −6.000 ± 0.089 −7.453 ± 0.131 3.95 ± 0.49 0.78 NGC 4382 129 186.33458 18.19567 1.03 −5.339 ± 0.116 −6.672 ± 0.221 3.49 ± 1.18 0.72 NGC 4382 131 186.33261 18.17919 1.36 −7.442 ± 0.041 −8.721 ± 0.031 2.50 ± 0.17 1.00 NGC 4382 132 186.33410 18.19102 1.01 −6.062 ± 0.109 −7.109 ± 0.085 3.08 ± 0.51 0.85 NGC 4382 133 186.33272 18.17975 1.33 −5.062 ± 0.578 −6.870 ± 0.279 4.03 ± 5.29 0.60 NGC 4382 135 186.33106 18.16635 2.03 −8.286 ± 0.046 −9.331 ± 0.036 6.78 ± 0.18 0.86 NGC 4382 136 186.33505 18.19753 1.04 −5.523 ± 0.080 −7.191 ± 0.106 4.33 ± 0.43 0.58 NGC 4382 138 186.33545 18.19987 1.09 −8.242 ± 0.055 −9.129 ± 0.021 2.34 ± 0.21 1.00 NGC 4382 140 186.33385 18.18673 1.07 −7.698 ± 0.020 −8.641 ± 0.031 2.48 ± 0.20 1.00 NGC 4382 142 186.33653 18.20678 1.34 −8.226 ± 0.021 −9.417 ± 0.016 2.86 ± 0.15 1.00 NGC 4382 148 186.33412 18.18479 1.09 −8.411 ± 0.027 −9.325 ± 0.029 4.13 ± 0.15 1.00 NGC 4382 151 186.33305 18.17528 1.50 −7.913 ± 0.022 −8.965 ± 0.023 2.71 ± 0.20 1.00 NGC 4382 152 186.33439 18.18539 1.06 −9.213 ± 0.013 −10.142 ± 0.023 3.80 ± 0.13 1.00 NGC 4382 154 186.33714 18.20703 1.33 −5.471 ± 0.474 −6.724 ± 0.116 3.73 ± 1.02 0.67 NGC 4382 155 186.33352 18.17839 1.34 −5.646 ± 0.233 −6.793 ± 0.146 3.47 ± 0.81 0.73 NGC 4382 156 186.33209 18.16708 1.95 −5.021 ± 0.372 −6.229 ± 0.563 2.18 ± 0.69 0.74 NGC 4382 157 186.33371 18.17944 1.29 −5.421 ± 0.149 −6.293 ± 0.187 4.02 ± 0.77 0.60 NGC 4382 161 186.33449 18.18314 1.12 −5.976 ± 0.091 −7.186 ± 0.140 3.54 ± 0.73 0.78 NGC 4382 162 186.33580 18.19281 0.91 −5.260 ± 0.453 −6.715 ± 0.220 3.71 ± 0.90 0.68 NGC 4382 167 186.33755 18.20369 1.15 −9.008 ± 0.021 −10.115 ± 0.027 2.98 ± 0.13 1.00 NGC 4382 169 186.33326 18.17046 1.73 −5.432 ± 0.511 −7.298 ± 0.222 3.99 ± 1.74 0.72 NGC 4382 171 186.33769 18.20466 1.19 −6.752 ± 0.047 −7.775 ± 0.047 2.03 ± 0.27 0.91 NGC 4382 176 186.33795 18.20490 1.19 −7.869 ± 0.026 −8.599 ± 0.039 3.78 ± 0.14 1.00 NGC 4382 177 186.33492 18.18145 1.15 −6.345 ± 0.051 −7.336 ± 0.049 2.29 ± 0.31 0.92 NGC 4382 178 186.33832 18.20801 1.34 −5.828 ± 0.063 −6.717 ± 0.155 3.32 ± 0.64 0.76 NGC 4382 179 186.33746 18.20118 1.04 −5.674 ± 0.144 −7.167 ± 0.307 3.36 ± 1.01 0.81 NGC 4382 181 186.33324 18.16784 1.87 −7.217 ± 0.040 −8.527 ± 0.034 3.68 ± 0.19 1.00 NGC 4382 190 186.33605 18.18676 0.93 −9.352 ± 0.016 −10.535 ± 0.013 2.61 ± 0.11 1.00 NGC 4382 192 186.33732 18.19634 0.88 −5.767 ± 0.085 −7.095 ± 0.115 3.62 ± 0.63 0.74 NGC 4382 193 186.33536 18.18053 1.16 −9.088 ± 0.018 −10.218 ± 0.018 2.82 ± 0.15 1.00 Continued on Next Page. . . 319
Page 1 and 2:
LOW-MASS X-RAY BINARIES, DIFFUSE GA
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smaller GCs are more likely to cont
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GO2-3099X, GO3-4099X, AR3-4005X, GO
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her room (my apologies to her offic
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US Court expert from India), for al
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Table of contents Abstract ii Ackno
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5.2.1 Chandra X-ray Observatory . .
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List of Figures 1.1 Hubble Tuning F
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List of Tables 1.1 Galactic Low-Mas
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Chapter 1 General Introduction 1.1
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Fig. 1.1.— Hubble Tuning Fork, co
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2000). In most HMXBs, the accreted
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not get a complete picture of the L
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this, the result of dynamical inter
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is the Advanced CCD Imaging Spectro
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Chapter 2 Chandra Observations of L
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keV (Sarazin et al. 2000, 2001). Wi
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agreed with positions from the USNO
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24:00 22:00 7:20:00 18:00 16:00 18:
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Table 2.1. Discrete X-ray Sources i
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Table 2.1—Continued Source d Coun
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Table 2.2—Continued Source d Coun
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optical/IR positions of R.A. = 12 h
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log N(>L) 2.0 1.5 1.0 0.5 0.0 NGC 4
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luminosity function for luminositie
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H31 1.0 0.5 0.0 -0.5 -1.0 NGC 4365
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2.4.5 Variability We searched for v
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Number 10 8 6 4 2 NGC 4365 Optical
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LMXBs has an effective radius of 12
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component (“MEKAL”) was used fo
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Table 2.4. X-ray Spectral Fits of N
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Fig. 2.9.— Top panels: Cumulative
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we extended the spectrum down to 0.
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We also examined whether the unreso
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esolved sources in the galaxy. This
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temperature ∼0.3 keV. Matsumoto e
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log I X (counts/sec/arcmin 2 ) -1.0
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∼45% of the counts are resolved i
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Chapter 3 Chandra Observations of D
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noninteracting members (de Vaucoule
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used for spectroscopic analysis. We
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02:00.0 03:00.0 04:00.0 05:00.0 06:
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Table 3.1—Continued d a Count Rat
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We also attempted detections in mul
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sociated with extended X-ray or opt
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Fig. 3.3.— Histogram of the obser
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chip. The number of ULX candidates
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these luminosities among previously
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to 2-6 keV. Since the 6-10 keV rang
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absorption and varying power-law in
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counts occur within ∼ 4 ks. Sourc
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log I X (counts/sec/arcmin 2 ) 0.5
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tion), and βouter = 0.36 +0.01 −
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the east and northeast of NGC 1600.
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group, we assumed that they were at
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the group gas than we calculate fro
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04:55 -5:05:00 05 -5:05:10 15 -5:05
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for the spectrum: “Field” impli
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90% confidence level errors. Bracke
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we adopted the power-law model as o
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sources could be a non-trivial sour
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jection to include the emission fro
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Fig. 3.13.— Estimated gas and gra
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ackground source population cannot
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NGC 1600 that has a small spatial s
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(HMXBs). LMC X-4, an HMXB pulsar, h
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searched for the shortest time tn o
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with NGC 4697. Columns (1)-(4) list
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duration, ∆tflat, beginning at a
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the uncertainties quoted do not inc
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to persistent rate for short flares
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Chapter 5 Multi-Epoch Chandra X-ray
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the field, these different populati
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luminous (MB < −20) elliptical (E
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Although Chandra is known to encoun
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42:00.0 44:00.0 46:00.0 48:00.0 -5:
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Fig. 5.3.— Adaptively smoothed Ch
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1 × 10 −5 count s −1 arcsec
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Table 5.1—Continued Source R.A. D
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source list against which to regist
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ate from Observation 0784 alone (Pa
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Table 5.2. : Optical Properties of
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actually be an AGN. Sources 79, 80,
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two potential GC counterparts. We l
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Table 5.3—Continued X-ray Source
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Fig. 5.6.— Color (G475−Z850) -
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mass segregation of GCs with the sa
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Table 5.4. Fits to the Expected Num
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dependence are allowed to vary. Var
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NGC 4697 to convert the observed so
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Table 5.6—Continued Source LA LB
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Table 5.6—Continued Source LA LB
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Table 5.7. Combined Luminosities &
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Table 5.7—Continued Source Not De
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Fig. 5.8.— Cumulative luminosity
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LF, there are enough datapoints tha
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Fig. 5.10.— Cumulative luminosity
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Fig. 5.11.— Merged luminosities (
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Fig. 5.12.— X-ray color-color dia
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5.9 Spectral Analysis We performed
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some data loss, it allows for direc
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for 2 dof and the f-test indicates
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ple to LMXBs interior to that semi-
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est-fit (χ 2 = 56.4 for 65 dof) by
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5.10.1 Intraobservation Variability
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Fig. 5.14.— Binned lightcurve usi
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Table 5.10. Possible Flaring Source
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Fig. 5.16.— Cumulative lightcurve
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pairs of observations. In Figure 5.
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Table 5.11—Continued Source PL,AB
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Fig. 5.17.— Percentage of Analysi
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dofs and the number of combinations
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Table 5.12—Continued Source Obs.S
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of states as transient candidates.
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Long-Term Hardness Ratio Variabilit
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In the final observation, there wer
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limits). The 0.3-10 keV X-ray lumin
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atio is expected only from the most
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eak (Kim et al. 2006a). We find mar
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LMXBs in Galactic GCs (Heinke et al
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in the field of the Milky Way and a
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6.2 Sample 6.2.1 Galaxy Sample Tabl
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Table 6.2. Properties of Chandra Ob
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identification of point sources, AC
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the QE degradation in the ACIS dete
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Table 6.3—Continued Galaxy NX LX,
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The positions of the GCs were used
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Fig. 6.2.— Scatter plot of GC gal
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Fig. 6.3.— Scatter plot of estima
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Fig. 6.5.— Scatter plot of estima
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isophote from the galaxy optical su
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6.3.1 Luminosity and Mass Prior obs
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compare their χ 2 fits to test whi
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GCs without LMXBs; however, there a
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following dependence on GC properti
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of this probability with individual
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Fig. 6.9.— Identical to Figure 6.
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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
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Table B.2—Continued RA Dec. d GC
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investigations into improving the h
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C.4 Sivakoff Signature Soy Sauce Sk
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Blanton, E. L., Sarazin, C. L., & I
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Frogel, J. A., Persson, S. E., Matt
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Johnston, H. M. & Verbunt, F. 1996,
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Makishima, K. et al. 2000, ApJ, 535
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Porter, A. C. 1993, PASP, 105, 1250
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Verner, D. A., Ferland, G. J., Kori
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