Table 1
Pulsars around HESS J1741−302 with their properties.
| Pulsar name | Position | τc | DPSR | Offset | Separation |  |
Ė/ |
 |
|---|---|---|---|---|---|---|---|---|
| (J2000) | (kyr) | (kpc) | (°) | (pc) | (erg/s) | (erg/s/kpc2) | (%) | |
| PSR B1737−30 | RA: 17h40m33.8s | 20.6 | 0.4 | 0.19 | 1.3 | 8.2 ×1034 | 5.1 ×1035 | 0.03 |
| Dec: −30°15′43.2′′ | 3.28 | 10.9 | 7.6 ×1033 | 1.84 | ||||
| PSR J1739−3023 | RA: 17h39m39.8s | 159 | 3.41 | 0.35 | 20.8 | 3.0 ×1035 | 2.6 ×1034 | 0.54 |
| Dec: −30°23′12.0′′ | ||||||||
Notes. Pulsar data were taken from Manchester et al. (2005). The position column indicates the positions of pulsars, while the columns
labeled τc
and DPSR
show the characteristic age and the pulsar dispersion measure distance, respectively. The offset and
separation columns show the relative offset of the pulsars with respect to the best fit position of
HESS J1741−302
and the corresponding physical separation for the given pulsar distances, respectively. The
Ė and
columns give the spin-down luminosity and flux of pulsars, respectively. The column labeled as
Lγ ∕Ė gives the
VHE γ-ray
efficiencies of pulsars.
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