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Table 5
Spitzer/GLIMPSE II and III and MSX magnitudes for bulge RCB stars.
Spitzer IRAC bands | MSX bands | |||||||
Name | [3.6] | [4.5] | [5.8] | [8.0] | A (8.26 μm) | C (12.12 μm) | D (14.65 μm) | E (21.41 μm) |
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Known RCB stars | ||||||||
EROS2-CG-RCB-1II | 5.388s | 4.645s | 3.765 | nd | 4.13 | 3.68 | 3.44 | nd |
EROS2-CG-RCB-3 | 6.648s | 5.164s | 4.372 | 3.662 | 3.40 | 2.81 | 2.59 | 2.33 |
EROS2-CG-RCB-4 | 6.712s | 5.546s | 4.361 | 3.695 | 4.25 | 3.66 | 3.30 | nd |
EROS2-CG-RCB-5 | 6.525s | 5.485s | 4.780 | 4.185 | 3.66 | 3.02 | 3.02 | nd |
EROS2-CG-RCB-6 | 7.406s | nd | 5.664 | 4.832 | 4.34 | 3.67 | 3.30 | nd |
EROS2-CG-RCB-7 | 7.119s | nd | 5.353 | 4.793 | 4.95 | nd | nd | nd |
EROS2-CG-RCB-8II | 7.019s | 6.310s | 5.281 | 4.519 | 4.46 | 3.96 | 3.71 | 3.69 |
EROS2-CG-RCB-9 | 6.605s | 6.109s | 4.699 | 3.935 | 3.90 | 3.15 | 2.76 | nd |
EROS2-CG-RCB-10 | 5.100s | 4.594s | 3.704 | 2.933 | 2.91 | 2.24 | 2.04 | 1.62 |
EROS2-CG-RCB-11 | 7.021s | 6.030s | 5.385 | 4.670 | 4.09 | 3.47 | 3.16 | nd |
EROS2-CG-RCB-13 | 6.849s | 6.122s | 4.869 | 4.159 | 4.31 | 3.57 | 3.87 | nd |
EROS2-CG-RCB-14o | nd | nd | nd | nd | 3.75 | 3.06 | 2.98 | nd |
MACHO-301.45783.9o | nd | nd | nd | nd | 5.06 | nd | nd | nd |
MACHO-308.38099.66 | 6.200s | 5.541s | 4.847 | 4.217 | nd | nd | nd | nd |
MACHO-401.48170.2237II | 6.702s | nd | 4.404 | 3.724 | nd | nd | nd | nd |
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Known DYPer type stars | ||||||||
EROS2-CG-RCB-2II | 8.167 | 7.893 | 7.667 | 7.367 | nd | nd | nd | nd |
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New RCB stars | ||||||||
OGLE-GC-RCB-1 | 6.449s | 5.932s | 4.813 | 4.116 | 4.55 | 3.99 | 3.73 | nd |
OGLE-GC-RCB-2II | 7.678s | 6.935s | 6.243 | 5.354 | 3.94 | 3.02 | 3.01 | 2.43 |
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New RCB star candidates | ||||||||
OGLE-GC-RCB-Cand-1II | 7.602 | 6.751 | 5.806 | 4.887 | 4.97 | 3.92 | 3.53 | 2.89 |
OGLE-GC-RCB-Cand-2 | 7.552s | 7.019s | 6.293 | 5.593 | 5.25 | nd | nd | nd |
GLIMPSE-RCB-Cand-1 | 6.789s | 5.822s | 5.030 | 4.447 | 5.05 | nd | 3.46 | nd |
GLIMPSE-RCB-Cand-2 | 6.062s | 5.239s | 4.505 | 3.890 | 3.45 | 2.76 | 2.68 | nd |
Notes. nd = not detected; s probably saturated, measurement can’t be trusted. IISpitzer magnitudes from GLIMPSE-II-Archive catalogues, instead of GLIMPSE-III-Archive for the others. o Located outside Spitzer GLIMPSE fields.
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