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Query : 2022A&A...658A..60Y |
2022A&A...658A..60Y - Astronomy and Astrophysics, volume 658A, 60-60 (2022/2-1)
Possible hadronic origin of TeV photon emission from SNR G106.3+2.7.
YANG C., ZENG H., BAO B. and ZHANG L.
Abstract (from CDS):
Abstract Copyright: © ESO 2022
Journal keyword(s): radiation mechanisms: non-thermal - ISM: supernova remnants - gamma rays: general
Simbad objects: 4
Number of rows : 4 |
N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2024 |
#notes |
---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | IC 443 | SNR | 06 17 00.0000000 | +22 34 11.998901 | ~ | 1235 | 1 | |||||
2 | SNR G034.6-00.5 | SNR | 18 56 10.650 | +01 13 21.30 | ~ | 964 | 2 | |||||
3 | SNR G106.3+02.7 | SNR | 22 27.5 | +60 50 | ~ | 76 | 1 | |||||
4 | PSR J2229+6114 | Psr | 22 29 05.262 | +61 14 08.48 | ~ | 221 | 2 |
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