| Canonical Name: | 3HWC J1739+099 |
| TeVCat Name: | TeV J1739+099 |
| Other Names: | 1LHAASO J1740+0948u |
| Source Type: | UNID |
| R.A.: | 17 39 58.3 (hh mm ss) |
| Dec.: | +09 55 49 (dd mm ss) |
| Gal Long: | 33.89 (deg) |
| Gal Lat: | 20.34 (deg) |
| Distance: | |
| Flux: | (Crab Units) |
| Energy Threshold: | GeV |
| Spectral Index: | |
| Extended: | No |
| Discovery Date: | 2020-12 |
| Discovered By: | HAWC |
| TeVCat SubCat: | Default Catalog |
Source Notes:
More details on this source from
The Third HAWC Catalog will soon be added to TeVCat.
Source Association:
From
Albert et al. (2020):
- From Table 3, "the nearest GeV source in 4FGL (
Abdollahi et al. 2020)
and its separation from the 3HWC source; the source class as listed in 4FGL
where available (bcu: active galaxy of uncertain type; PSR: pulsar, identified
by pulsations; unk: unknown); the nearest pulsar and corresponding separation
from the ATNF pulsar catalog (
Manchester et al. 2005); and the nearest
SNR, separation distance, and type from the SNRCat (
Ferrand & Safi-Harb 2012).":
- 4FGL J1740.5+1005, 0.22 deg, PSR
- J1740+1000, 0.13 deg
- G034.0+20.3, 0.13 deg, filled-centre
A PeVatron:
From
Cao et al. (2024):
- This source is listed as being a UHE source in Table 2. This means
that it has a detection above 100 TeV at a significance level
corresponding to a test statistic of greater than 20.
Seen by: HAWC, LHAASO
-
Ultra-high-energy gamma-ray emission associated with the tail of a bow-shock pulsar wind nebula
Cao, Zhen et al., arXiv e-prints parXiv:2502.15447 (2025) [LINK]
-
The First LHAASO Catalog of Gamma-Ray Sources
Cao, Zhen et al., ApJS 271 p25 (2024) [LINK]
-
3HWC: The Third HAWC Catalog of Very-high-energy Gamma-Ray Sources
Albert, A. et al., ApJ 905 p76 (2020) [LINK]
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