| Canonical Name: | 0FGL J0631.8+1034 |
| TeVCat Name: | TeV J0631+105 |
| Other Names: | J0631+10 |
| Source Type: | PWN |
| R.A.: | 06 31 49.22 (hh mm ss) |
| Dec.: | +10 34 12.7 (dd mm ss) |
| Gal Long: | 201.30 (deg) |
| Gal Lat: | 0.51 (deg) |
| Distance: | 6.55 kpc |
| Flux: | 0.29 (Crab Units) |
| Energy Threshold: | 3500 GeV |
| Spectral Index: | |
| Extended: | No |
| Discovery Date: | 2009-04 |
| Discovered By: | Milagro |
| TeVCat SubCat: | Source Candidates |
Source Notes:
Milagro report a source associated with 0FGL J0631.8+1034 with a
statistical significance of 3.7sigma.
The flux quoted here is based on a comparison of the quoted Milagro
flux at 35 TeV of 47.2e-17 /TeV /s /cm2 with that from the Crab
(162.6e-17 /TeV /s /cm2) also quoted at 35 TeV.
This source is associated with a Fermi pulsar and is therefore
postulated to be the PWN of this pulsar (
Abdo et al. 2009)
Seen by: Milagro
-
MAGIC observations on Pulsar Wind Nebulae around high spin-down power Fermi-LAT pulsars
Fern et al., ArXiv e-prints p (2017) [LINK]
-
Milagro Observations of TeV Emission from Galactic Sources in the Fermi Bright Source List
Abdo, A.A. et al., ArXiv e-prints p (2009) [LINK]
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