| Canonical Name: | LHAASO J2032+4102 |
| TeVCat Name: | TeV J2032+410 |
| Other Names: | TeV J2032+4130
2HWC J2031+415
VER J2032+414
ARGO J2031+4157
MGRO J2031+41
Cygnus OB2
PSR J2032+4127
SNR G79.8+1.2 |
| Source Type: | UNID |
| R.A.: | 20 32 12 (hh mm ss) |
| Dec.: | +41 03 00 (dd mm ss) |
| Gal Long: | 79.89 (deg) |
| Gal Lat: | 0.79 (deg) |
| Distance: | |
| Flux: | 0.54 (Crab Units) |
| Energy Threshold: | 100000 GeV |
| Spectral Index: | |
| Extended: | Yes |
| Size (X): | 0.00 (deg) |
| Size (Y): | 0.00 (deg) |
| Discovery Date: | 2021-05 |
| Discovered By: | LHAASO |
| TeVCat SubCat: | Default Catalog |
Source Notes:
Details of the source detection:
From
Cao et al. (2021):
- "At 100 TeV, the angular and energy resolutions are about 15–20 arcmin
and better than 20%, respectively, allowing adequate spectroscopic and
morphological studies."
- "The statistical significance of the detection above 100 TeV is calculated
using a 0.3deg extension template"
- "Crab Units (CU), flux of the Crab Nebula at 100 TeV; 1 CU = 6.1 x 10-17 photons TeV-1 cm-2 s-1)"
- Significance above 100 TeV: 10.5 sigma
- E_max (PeV): 1.42 +/- 0.13
- Differential photon flux at 100 TeV (CU): 0.54 +/- 0.10
- On-source events/Off-source events: 45/6.7
- Exposure (hr): 2648.2.
Source Position:
From
Cao et al. (2021):
- R.A. (J2000): 308.05 = 20h 32m 12s
- Dec. (J2000): +41.05 = +41d 03m
Possible Origin:
From
Cao et al. (2021):
- This list contains sources potentially at the origin of the LHAASO source, together with their class, their distance, age and luminosity
- Cygnus OB2, Young Molecular Cloud, Distance: 1.40 +/- 0.08 kpc
- PSR J2032+4127, Pulsar, Distance: 1.40 +/- 0/08 kpc, Age: 201 kyr, L_s: 1.5 x10e35
- SNR G79.8+1.2, Supernova Candidate
Potential TeV Counterparts:
From
Cao et al. (2021):
- This list contains "Nearby teraelectronvolt sources within 1deg of the centre of the LHAASO source"
-
TeV J2032+4130 / 2HWC J2031+415 / VER J2032+414
-
ARGO J2031+4157
-
MGRO J2031+41
Pevatron:
From
Mitchell (2021):
- this source is included in a list of Galactic sources currently known
to produce gamma-ray emission above 100 TeV.
Seen by: LHAASO
-
PeV proton acceleration in Gamma-ray Binaries
Bykov, A.M. et al., arXiv e-prints parXiv:2401.06271 (2024) [LINK]
-
Modeling of GeV-TeV gamma-ray emission of Cygnus Cocoon
Bykov, A.M. and Kalyashova, M.E., arXiv e-prints parXiv:2203.09842 (2022) [LINK]
-
Limits on Leptonic TeV Emission from the Cygnus Cocoon with Swift-XRT
Guevel, David et al., arXiv e-prints parXiv:2211.07617 (2022) [LINK]
-
Ultrahigh-energy photons up to 1.4 petaelectronvolts from 12 gamma-ray Galactic sources
Cao, Z., Aharonian, F.A., An, Q., et al., Nature 594 p33-36 (2021) [LINK]
-
Strong constraints on Lorentz violation using new gamma-ray observations around PeV
Chen, Liang et al., arXiv e-prints parXiv:2105.07927 (2021) [LINK]
-
Constraints on Hadronic Contribution to LHAASO Sources with Neutrino Observations
Huang, Tian-Qi and Li, Zhuo, arXiv e-prints parXiv:2105.09851 (2021) [LINK]
-
Ultrahigh-energy photons from LHAASO as probes of Lorentz symmetry violations
Li, Chengyi and Ma, Bo-Qiang, arXiv e-prints parXiv:2105.07967 (2021) [LINK]
-
Status of Ground-based and Galactic Gamma-ray Astronomy
Mitchell, A.M.W., arXiv e-prints parXiv:2109.13753 (2021) [LINK]
-
The Hunt for Pevatrons: The Case of Supernova Remnants
Cristofari, P., arXiv e-prints parXiv:2110.07956 (2021) [LINK]
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