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

Table 6.3—Continued
Galaxy NX LX,min a NGCs (g − z)div NBlue GCs NRed GCs NGCs w LMXBs NBlue GCs w LMXBs NRed GCs w LMXBs NFalse Matches
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)
Complete: All Sources with Luminosities > 3.2 × 1038 erg s−1 NGC 4365 19 3.20 907 1.160 418 [1] 489 [5] 10 (3) 1 (0) 8 (2) 0.93
NGC 4374 12 3.20 506 1.200 310 [0] 196 [0] 4 (0) 2 (0) 2 (0) 0.45
NGC 4382 9 3.20 505 1.230 320 [0] 185 [0] 1 (0) 1 (0) 0 (0) 0.43
NGC 4406 16 3.20 367 1.220 260 [0] 107 [0] 5 (0) 3 (0) 2 (0) 0.38
NGC 4472 19 3.20 764 1.180 306 [0] 458 [2] 9 (1) 0 (0) 9 (1) 0.62
NGC 4486 27 3.20 1639 1.190 690 [3] 949 [5] 14 (3) 2 (0) 10 (1) 2.26
NGC 4526 4 3.20 244 1.170 121 [0] 123 [0] 1 (0) 1 (0) 0 (0) 0.11
NGC 4552 17 3.20 456 1.190 217 [1] 239 [1] 10 (1) 3 (0) 6 (0) 0.45
NGC 4621 7 3.20 308 1.110 121 [0] 187 [0] 2 (0) 0 (0) 2 (0) 0.23
NGC 4649 20 3.20 807 1.200 335 [0] 472 [0] 10 (0) 2 (0) 8 (0) 0.54
NGC 4697 3 3.20 298 1.127 127 [0] 171 [0] 3 (0) 0 (0) 3 (0) 0.00
a Units are 1038 erg s−1 in 0.3–10 keV band.
b If an X-ray source was within 1 ′′ of GCs and non-GC sources, it is unclear if the X-ray source is matched to a GC; the possibly matching GCs have
been removed from this sample. Numbers in brackets indicate the number of GCs where (only) multiple GCs are within 1 ′′ of an X-ray source.
c The number of RGC-LMXBs and BGC-LMXBs will not add up to the number of GC-LMXBs if an X-ray source is within 1 ′′ of both an RGC and a
BGC. Numbers in parenthesis indicate the number of X-ray sources where (only) multiple GCs are within 1 ′′ of an X-ray source.
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