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Query : 2004ApJ...601..340K |
2004ApJ...601..340K - Astrophys. J., 601, 340-351 (2004/January-3)
The most likely sources of high-energy cosmic-ray electrons in supernova remnants.
KOBAYASHI T., KOMORI Y., YOSHIDA K. and NISHIMURA J.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): Acceleration of Particles - ISM: Cosmic Rays - Gamma Rays: Theory - ISM: Supernova Remnants
CDS comments: In the introd. G374.3-0.5 is a misprint for G347.3-0.5 (= SNR 347.3-0.5)
Simbad objects: 17
Number of rows : 17 |
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 | 1FGL J0538.6+2717 | BL? | 05 39 00.000 | +27 50 00.00 | ~ | 253 | 2 | |||||
2 | IC 443 | SNR | 06 17 00.0000000 | +22 34 11.998901 | ~ | 1235 | 1 | |||||
3 | NAME Geminga | Psr | 06 33 54.153 | +17 46 12.91 | ~ | 1222 | 0 | |||||
4 | NAME MONOGEM SNR | SNR | 06 58 50 | +13 55.9 | ~ | 104 | 0 | |||||
5 | NAME Vela X | Psr | 08 33 08.880 | -45 11 24.36 | ~ | 281 | 1 | |||||
6 | NAME Vela XYZ | Rad | 08 34.0 | -45 50 | ~ | 1230 | 2 | |||||
7 | NAME Vela Pulsar | Psr | 08 35 20.65525 | -45 10 35.1545 | 15.10 | ~ | 2315 | 1 | ||||
8 | NAME Vela Jr SN | BL? | 08 52.0 | -46 20 | ~ | 474 | 2 | |||||
9 | ESO 134-11 | HII | 14 40 29 | -62 38.7 | ~ | 565 | 1 | |||||
10 | 1A 1439-61 | BL? | 14 43 00 | -62 30.0 | ~ | 368 | 1 | |||||
11 | NAME Loop I | SR? | 15 01 | -38.7 | ~ | 387 | 2 | |||||
12 | NAME Lupus SN | SNR | 15 02 22.1 | -42 05 49 | ~ | 1328 | 1 | |||||
13 | 1FGL J1711.7-3944c | BL? | 17 12 27 | -39 41.2 | 12.27 | ~ | 723 | 1 | ||||
14 | SNR G065.2+05.7 | SNR | 19 33.0 | +31 10 | ~ | 101 | 0 | |||||
15 | SNR G089.0+04.7 | SNR | 20 45.0 | +50 35 | ~ | 224 | 0 | |||||
16 | NAME Cyg Loop | SNR | 20 51.0 | +30 40 | ~ | 913 | 0 | |||||
17 | 3C 461 | BL? | 23 23 24.000 | +58 48 54.00 | 14.30 | ~ | 2792 | 1 |
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