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Query : 2003ApJ...596L..75S |
2003ApJ...596L..75S - Astrophys. J., 596, L75-L78 (2003/October-2)
Can the age discrepancies of neutron stars be circumvented by an accretion-assisted torque.
SHI Y. and XU R.X.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): Stars: Pulsars: General - Stars: Pulsars: Individual: Alphanumeric: 1E 1207.4-5209 - Stars: Neutron
CDS comments: Parag. 1 : 1E 2259+568 is a misprint for 1E 2259+586
Simbad objects: 15
Number of rows : 15 |
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 | M 1 | SNR | 05 34 30.9 | +22 00 53 | ~ | 6193 | 1 | |||||
2 | V* CM Tau | Psr | 05 34 31.9474694616 | +22 00 52.153698024 | ~ | 5261 | 0 | |||||
3 | 2E 2336 | HXB | 10 50 08.93 | -59 53 19.9 | Be | 405 | 0 | |||||
4 | AJG 14 | BL? | 12 09 40 | -52 25.0 | ~ | 287 | 1 | |||||
5 | PSR J1210-5226 | Psr | 12 10 00.88 | -52 26 28.4 | ~ | 225 | 1 | |||||
6 | PSR J1708-4008 | Psr | 17 08 49.0 | -40 09 10 | ~ | 293 | 0 | |||||
7 | PSR B1757-24 | Psr | 18 01 00.016 | -24 51 27.50 | ~ | 244 | 1 | |||||
8 | NAME Duck Redux | Rad | 18 02 10.000 | -24 54 00.00 | ~ | 179 | 3 | |||||
9 | SNR G011.2-00.3 | SNR | 18 11 28.9 | -19 25 29 | ~ | 286 | 1 | |||||
10 | PSR J1811-1926 | Psr | 18 11 29.15 | -19 25 25.4 | ~ | 126 | 1 | |||||
11 | SNR G011.2-01.1 | SNR | 18 14.0 | -19 46 | ~ | 66 | 1 | |||||
12 | SNR G029.7-00.2 | SNR | 18 46 22.8 | -02 59 47 | ~ | 350 | 2 | |||||
13 | PSR J1846-0258 | Psr | 18 46 24.94 | -02 58 30.1 | ~ | 347 | 2 | |||||
14 | 2E 4673 | HXB | 23 01 08.14 | +58 52 44.5 | ~ | 633 | 1 | |||||
15 | CTB 109 | BL? | 23 01 35 | +58 53.0 | ~ | 344 | 0 |
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