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Table 10

Summary of results on HMXB spectral type (SpT) presented in this study.

Source NIR Counterpart RA (J2000) NIR Counterpart Dec (J2000) Previous identification Derived SpT (this paper)

IGR J10101-5654 10:10:11.87 –56:55:32.1 HMXB ? (1,2) sgB[e]
IGR J11187-5438 11:18:21.21 –54:37:28.6 ? LMXB ?
IGR J11435-6109 11:44:00.30 –61:07:36.5 B2III or B0V (3) B0.5Ve
IGR J13020-6359 13:01:58.7 –63:58:09.0 Be (4) B0.5Ve
IGR J14331-6112 14:33:08.33 –61:15:39.7 BIII or BV, Be ? (5) Be ?
IGR J14488-5942 14:48:43.33 –59:42:16.3 Be ? (6) Oe/Be
IGR J16195-4945 16:19:32.20 –49:44:30.5 O/B supergiant (7) ON9.7Iab
IGR J16318-4848 16:31:48.31 –48:49:00.7 sgB[e] (8) sgB[e]
IGR J16320-4751 16:32:01.75 –47:52:28.9 O supergiant ? (9,10) BN0.5Ia
IGR J16328-4726 16:32:37.91 –47:23:40.9 O/B supergiant ? (11) O8Iafpe
IGR J16418- 4532 16:41:50.79 –45:32:25.3 O/B supergiant (12) BN0.5Ia
IGR J17200-3116 17:20:06.1 –31:17:02.0 HMXB ? (2) ?
IGR J17354-3255 17:35:27.60 –32:55:54.40 sgHMXB ? (13) O9Iab
IGR J17404-3655 17:40:26.85 –36:55:37.6 LMXB ? / HMXB ? (3,14) Be ?
IGR J17586-2129 17:58:34.56 –21:23:21.53 HMXB ? (14) supergiant O/B

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