2003ApJ...596L..75S


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):

It is found that 1E 1207.4-5209 could be a low-mass bare strange star if its small radius or low-altitude cyclotron formation can be identified. The age problems of five sources could be solved by a fossil-disk-assisted torque. The magnetic dipole radiation dominates the evolution of PSR B1757-24 at present, and the others are in propeller (or tracking) phases.

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

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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 - 2026
#notes
1 M 1 SNR 05 34 31.8 +22 01 03           ~ 6516 1
2 V* CM Tau Psr 05 34 31.9474694616 +22 00 52.153698024           ~ 5476 0
3 2E 2336 HXB 10 50 08.93 -59 53 19.9           Be 419 0
4 SNR G295.5+09.7 SNR 12 09 40 -52 25.0           ~ 301 1
5 PSR J1210-5226 Psr 12 10 00.88 -52 26 28.4           ~ 230 1
6 PSR J1708-4008 Psr 17 08 46.1 -40 08 56           ~ 315 0
7 PSR B1757-24 Psr 18 01 00.016 -24 51 27.50           ~ 258 1
8 NAME Milne 56 SNR 18 02 10.000 -24 54 00.00           ~ 182 3
9 SNR G011.2-00.3 SNR 18 11 28.9 -19 25 29           ~ 305 1
10 PSR J1811-1926 Psr 18 11 29.15 -19 25 25.4           ~ 136 1
11 SNR G011.2-01.1 SNR 18 14.0 -19 46           ~ 70 1
12 SNR G029.7-00.3 SNR 18 46 22.8 -02 59 47           ~ 375 2
13 PSR J1846-0258 Psr 18 46 24.75 -02 58 29.6           ~ 388 2
14 2E 4673 HXB 23 01 08.14 +58 52 44.5           ~ 673 1
15 SNR G109.1-01.0 SNR 23 01 35 +58 53.0           ~ 362 0

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