A study of the association of Fermi sources with massive young galactic objects

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Table 4

Positional coincidence of Fermi sources with WR stars.

Fermi name

Dec

95% Semi

Flux(E > 100 MeV)

Star

Dec

Δθ

Distance

(1FGL)

major axis (°)

(F ∝ E^− Γ)

× 10^-10 erg cm^-2 s^-1

(kpc)

J1745.6-2900

266.420

−29.014

0.019

2.26 ± 0.03

7.1 ± 0.7

WR 101a¹

266.41454

−29.00950

0.01

8.0

J1746.4-2849

266.618

−28.818

0.10

2.2 ± 0.5

4.6 ± 0.0

WR 102c²

266.54667

−28.81822

0.06

8.0

Notes.

⁽¹⁾

WR stars 101 b, c, d, e, f, g, h, i, j, k, l, m, n, o, belonging to the Galactic Center Cluster lie at distances less than 20′′ and are also within the error box of the gamma-ray source;

⁽²⁾

WR stars 102 d, e, f, g, h, i, j, k belonging to the Quintuplet Cluster lie at distances less than 1′ and are also coincident with the gamma-ray source.

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