2001ApJ...547..967S


Query : 2001ApJ...547..967S

2001ApJ...547..967S - Astrophys. J., 547, 967-972 (2001/February-1)

Implications of the optical observations of isolated neutron stars.

SHEARER A. and GOLDEN A.

Abstract (from CDS):

We show that observations of pulsars with pulsed optical emission indicate that the peak flux scales according to the magnetic field strength at the light cylinder. The derived relationships indicate that the emission mechanism is common across all of the observed pulsars with periods ranging from 33 to 385 ms and ages of 1000-300,000 yr. It is noted that similar trends exist for γ-ray pulsars. Furthermore, the model proposed by Pacini and developed by Pacini and Salvati still has validity and gives an adequate explanation of the optical phenomena.

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Journal keyword(s): Stars: Pulsars: General - Stars: Magnetic Fields - Stars: Neutron

Simbad objects: 17

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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 - 2026
#notes
1 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 19090 0
2 M 1 SNR 05 34 31.8 +22 01 03           ~ 6516 1
3 V* CM Tau Psr 05 34 31.9474694616 +22 00 52.153698024           ~ 5476 0
4 PSR J0537-6910 Psr 05 37 46.66 -69 10 17.1           ~ 309 1
5 PSR B0540-69 Psr 05 40 11.2000490438 -69 19 54.198559829           ~ 976 3
6 PSR J0633+1746 Psr 06 33 54.153 +17 46 12.91           ~ 1308 0
7 PSR B0656+14 Psr 06 59 48.18800 +14 14 19.2000   24.85 24.90     ~ 943 1
8 NAME Vela Pulsar Psr 08 35 20.65525 -45 10 35.1545     15.10     ~ 2446 1
9 PSR B0950+08 Psr 09 53 09.31210 +07 55 36.9000           ~ 806 2
10 PSR B1055-52 Psr 10 57 59.0450 -52 26 56.330           ~ 757 0
11 PSR B1706-44 Psr 17 09 42.62000 -44 29 12.0000     13.30     ~ 670 1
12 PSR J1824-2452A Psr 18 24 32.009 -24 52 11.10           ~ 529 2
13 M 28 GlC 18 24 32.89 -24 52 11.4           ~ 821 0
14 SNR G027.3+00.0 SNR 18 41 17.8 -04 56 12           ~ 345 3
15 PSR B1929+10 Psr 19 32 14.0570 +10 59 33.380           ~ 801 0
16 PSR B1951+32 Psr 19 52 58.181 +32 52 40.98           ~ 615 2
17 PSR J2322+2057 Psr 23 22 22.320041 +20 57 02.50080           ~ 129 1

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