Table 3
Positional coincidence of Fermi sources with MYSOs.
Fermi Name | RA | Dec | 95% Semi | Spectral index Γ | Flux(E > 100 MeV) | MSX name | RA | Dec | Δθ | Distance* | Lbol* | Mass | ||
(1FGL) |
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major axis (°) | (F ∝ E − Γ) | × 10-11 erg cm-2 s-1 |
![]() |
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(kpc) |
![]() |
(M⊙) | |||
|
||||||||||||||
J0541.1+3542 | 85.2805 | 35.7091 | 0.1397 | 2.41 ± 0.13 | 1.6 ± 0.5 | G173.6328 + 02.8064 | 85.27929 | + 35.82633 | 0.12 | 1.6a | 4.8d | |||
G173.6339 + 02.8218 | 85.29592 | + 35.83380 | 0.13 | 1.6a | 3.2e | |||||||||
G173.6882 + 02.7222 | 85.22758 | + 35.73558 | 0.05 | 1.6a | – | |||||||||
J0647.3+0031 | 101.8417 | 0.5289 | 0.2150 | 2.41 ± 0.11 | 1.9 ± 0.5 | G212.0641−00.7395 | 101.80567 | + 0.43514 | 0.10 | 6.4b | 25f | |||
J1256.9−6337 | 194.2474 | −63.6212 | 0.1955 | 2.26 ± 0.12 | 4.9 ± 1.1 | G303.5990 − 00.6524 | 194.35546 | −63.51650 | 0.12 | 11.3b | 8.3f | |||
J1315.0−6235 | 198.7635 | −62.5971 | 0.1860 | 2.31 ± 0.12 | 6.9 ± 0.0 | G305.4840 + 00.2248 | 198.40016 | −62.53708 | 0.18 | 3.6b | 3.8f | |||
J1651.5−4602 | 252.8831 | −46.0340 | 0.2258 | 2.21 ± 0.07 | 13.9 ± 3.4 | G339.8838 − 01.25881 | 253.01942 | −46.14267 | 0.14 | 2.6b | 21.0f | |||
J1702.4−4147 | 255.6039 | −41.7859 | 0.0800 | 2.39 ± 0.07 | 8.7 ± 2.0 | G344.4257 + 00.0451B | 255.53674 | −41.78303 | 0.05 | 5.0b | 15.0f | |||
G344.4257 + 00.0451C | 255.53587 | −41.78617 | 0.05 | 5.0b | 15.0f | |||||||||
J1846.8−0233 | 281.7001 | −2.5628 | 0.1262 | 2.21 ± 0.06 | 9.3 ± 2.3 | G030.1981 − 00.1691 | 281.76274 | −2.51003 | 0.08 | 7.4b | 29.0f | |||
J1848.1−0145 | 282.0470 | −1.7605 | 0.0859 | 2.23 ± 0.04 | 9.5 ± 3.2 | G030.9726−00.1410 | 282.09178 | −1.80842 | 0.07 | 5.7b | 3.9f | 1.9 × 103g | ||
G030.9959−00.0771 | 282.04516 | −1,75808 | 0.0044 | 5.7b | 5.1f | 1.9 × 103g | ||||||||
J1853.1+0032 | 283.2884 | 0.5366 | 0.5207 | 2.18 ± 0.07 | 5.7 ± 1.7 | G032.8205 − 00.3300 | 282.04436 | −1.75703 | 0.34 | 5.1b | 17.0f | |||
G033.3891 + 00.1989 | 282.89092 | + 0.49750 | 0.40 | 5.1b | 11.0f | |||||||||
G033.3933 + 00.0100 | 283.06109 | + 0.41528 | 0.26 | 6.8b | 7.9e | |||||||||
G033.5237 + 00.0198 | 283.11179 | + 0.53569 | 0.34 | 6.8b | 7.9e | |||||||||
G034.0126 − 00.2832 | 283.60437 | + 0.83239 | 0.43 | 13.3b | 34.0f | |||||||||
G034.0500 − 00.2977 | 283.63454 | + 0.85914 | 0.47 | 13.3b | 24.0f | |||||||||
J1925.0+1720 | 291.2748 | 17.3485 | 0.1443 | 2.28 ± 0.12 | 2.4 ± 1.0 | G052.2025 + 00.7217A | 291.24933 | + 17.42169 | 0.08 | 10.2b | 15.0f | |||
G052.2078 + 00.6890 | 291.28553 | + 17.41317 | 0.07 | 10.2b | 20.0f | |||||||||
J1943.4+2340 | 295.8667 | 23.6815 | 0.1118 | 2.23 ± 0.11 | 2.6 ± 0.7 | G059.7831 + 00.06482,3 | 295.79680 | + 23.73433 | 0.08 | 2.2a | 6.8f | 840 and 190 5 | ||
J2040.0+4157 | 310.0154 | 41.9533 | 0.1970 | 2.66 ± 0.06 | 7.9 ± 1.2 | G081.5168 + 00.1926 | 309.99066 | + 41.98739 | 0.04 | 1.7c | 0.704f |
Notes. Distances: Luminosities: Masses: .
Observed in the X-ray with Chandra (Beuther et al. 2002a).
MSX 21 μm band flux using a scaling relationship determined from a comparison with sources where spectral energy distribution (SED) fits have been possible;
SED fit to the available infrared fluxes (2MASS, MSX, MIPSGAL/IGA) and literature (sub)millimetre fluxes;
Data obtained from http://www.ast.leeds.ac.uk/cgi-bin/RMS/RMS_DATABASE.cgi;
from Ragan et al. (2006);
mass of the 2 cores identified in Beuther et al. (2002b)
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