A Tables of Binary and Millisecond Pulsars



PSR	$P$	$log t c$	$logB$	$d$	$v t$	Refs.
	[ms]	[ $log(yr)$ ]	[ $log(G)$ ]	[kpc]	[km/s]



J0030+0451	4.865	9.9	8.3	0.23	$< 65$	[177 ]
J0609+2130	55.698	9.6	9.56	1.20	?	[188 , 190 ]
J0711 $-$ 6830	5.491	10.4	8.2	1.04	139	[23 , 320 ]
J1024 $-$ 0719	5.162	9.7	8.5	0.35	45	[23 , 320 ]
J1629 $-$ 6902	6.000	10.0	8.4	1.36	?	[91 ]

J1721 $-$ 2457	3.497	10.0	8.2	1.56	?	[91 ]
J1730 $-$ 2304	8.123	9.9	8.6	0.51	53	[189 , 320 ]
J1744 $-$ 1134	4.075	9.9	8.3	0.17	20	[23 , 320 ]
J1801 $-$ 1417	3.625	10.0	8.1	1.80	?	[94 ]
J1843 $-$ 1113	1.846	9.5	8.1	1.97	?	[123 ]

B1937+21	1.558	8.4	8.6	9.65	22	[19 , 155 ]
J1944+0907	5.185	9.7	8.5	1.8	?	[217 ]
J2124 $-$ 3358	4.931	9.9	8.4	0.25	67	[23 , 320 ]
J2235+1506	59.767	10.0	9.4	1.15	98	[55 ]
J2322+2057	4.808	10.2	8.2	0.78	89	[240 , 56 ]

Table 2:

Parameters for the 15 isolated millisecond pulsars currently known in the Galactic disk. Two of the pulsars (J0609+2130 and J2235+1506) are thought to be the descendants of high-mass binary systems. Listed are the spin period $P$ , the base-10 logarithms of the characteristic age $tc$ and surface magnetic field strength $B$ (see Section 2.2), the distance $d$ derived from the Cordes & Lasio electron density model [73 , 74 ] or independently (when available), and the transverse speed $vt$ inferred from $d$ and a proper motion measurement (when available). Key publications for each pulsar are referenced to the bibliography.



PSR	$P$	$logtc$	$log B$	$d$	$vt$	$Pb$	$x$	$e$	$m2$	Refs.
	[ms]	[ $log(yr)$ ]	[ $log(G)$ ]	[kpc]	[km/s]	[days]	[s]		[ $Mo .$ ]



J0045 $-$ 7319	926.276	6.5	12.3	57.00	?	51.2	174.3	0.81	8.8	[30 ]
J0737 $-$ 3039A	22.699	8.3	9.8	0.57	?	0.1	1.4	0.088	1.25	[44 , 198 ]
J0737 $-$ 3039B	2773.46	7.7	12.2	0.57	?	0.1	1.5	0.088	1.34	[44 , 198 ]
J1141 $-$ 6545	393.898	6.2	12.1	3.20	115	0.20	1.86	0.17	1.0	[154 , 241 ]
B1259 $-$ 63	47.762	5.5	11.5	4.60	?	1237	1296	0.87	10.0	[139 , 140 ]

J1518+4904	40.935	10.3	9.0	0.70	27	8.63	20.04	0.25	1.3	[237 , 238 ]
B1534+12	7.904	8.4	10.0	0.68	80	0.42	3.73	0.27	1.3	[343 , 293 ]
J1638 $-$ 4715	764	?	?	?	?	1830	?	0.9	$> 4.5$	[193 ]
J1740 $-$ 3052	570.309	5.5	12.6	10.8	?	231	756.9	0.58	16	[295 , 296 ]
J1756 $-$ 2251	28.462	8.6	9.7	2.5	?	0.32	2.8	0.18	1.2	[93 ]

J1811 $-$ 1736	104.182	8.9	10.1	5.94	?	18.77	34.78	0.83	0.7	[199 ]
B1820 $-$ 11	279.828	6.5	11.8	6.26	?	357.8	200.7	0.79	0.7	[207 , 253 ]
J1829+2456	41.010	10.1	9.2	0.75	?	1.18	7.24	0.14	1.3	[62 , 61 ]
B1913+16	59.030	8.0	10.4	7.13	100	0.32	2.34	0.62	1.4	[312 , 313 ]
B2303+46	1066.371	7.5	11.9	4.35	?	12.34	32.69	0.66	1.2	[195 , 332 ]

Table 3:

Parameters for the 15 eccentric ( $e > 0.05$ ) binary pulsars currently known that are not in globular clusters. In addition to the parameters listed in Table 2, we also give the binary period $P b$ , the projected semi-major axis of the orbit $x$ in units of light seconds, the orbital eccentricity $e$ , and the companion mass $m2$ evaluated from the mass function assuming a pulsar mass of $1.4Mo .$ and an inclination angle of 60 degrees (see Section 4.4) or (when known) from independent measurements.


PSR	$P$	$log tc$	$log B$	$d$	$vt$	$Pb$	$x$	$e$	$m2$	Refs.
	[ms]	[ $log(yr)$ ]	[ $log(G)$ ]	[kpc]	[km/s]	[days]	[s]		[ $Mo .$ ]



J0034 $-$ 0534	1.877	9.9	7.9	0.98	71	1.59	1.44	$< 0.00002$	0.1	[22 ]
J0218+4232	2.323	8.7	8.6	5.85	?	2.03	1.98	$< 0.00002$	0.2	[235 ]
J0407+1607	25.702	9.7	9.2	1.30	35	669.1	106.5	0.000937	0.2	[190 ]
J0437 $-$ 4715	5.757	9.7	8.5	0.18	121	5.74	3.37	0.000019	0.1	[138 ]
J0613 $-$ 0200	3.062	9.7	8.2	2.19	77	1.20	1.09	0.000007	0.1	[189 , 320 ]

J0621+1002	28.854	10.1	9.0	1.88	?	8.31	12.03	0.0025	0.5	[57 ]
B0655+64	195.671	9.7	10.1	0.48	32	1.03	4.13	0.000008	0.7	[141 , 331 ]
J0751+1807	3.479	9.8	8.2	2.02	?	0.26	0.40	$> 0.0$	0.1	[192 ]
B0820+02	864.873	8.1	11.5	1.43	35	1232.47	162.15	0.011868	0.2	[212 , 331 ]
J1012+5307	5.256	9.8	8.4	0.52	102	0.60	0.58	$< 0.0000008$	0.1	[236 , 167 ]

J1022+1001	16.453	9.8	8.9	0.60	$> 50$	7.81	16.77	0.000098	0.7	[57 , 164 ]
J1045 $-$ 4509	7.474	10.0	8.5	3.25	52	4.08	3.02	0.000024	0.2	[189 , 320 ]
J1157 $-$ 5114	43.589	9.7	9.4	1.88	?	3.51	14.29	0.00040	1.2	[90 ]
J1232 $-$ 6501	88.282	9.2	9.9	10.00	?	1.86	1.61	0.00011	0.1	[54 ]
B1257+12	6.219	9.5	8.6	0.62	281	planetary system				[346 , 344 ]

J1420 $-$ 5625	34.117	9.9	9.2	1.74	?	40.3	29.5	0.0035	0.4	[123 ]
J1435 $-$ 6100	9.348	9.8	8.7	3.25	?	1.35	6.18	0.00001	0.9	[54 ]

J1454 $-$ 5846	45.249	9.0	9.8	3.32	?	12.42	26.52	0.0019	0.9	[54 ]
J1455 $-$ 3330	7.987	9.9	8.5	0.74	100	76.17	32.36	0.000170	0.3	[189 , 320 ]
J1603 $-$ 7202	14.842	10.2	8.7	1.64	27	6.31	6.88	$> 0.0$	0.3	[187 , 320 ]

J1618 $-$ 39	11.987	?	?	4.76	?	22.8	10.2	0.0	0.2	[91 ]
J1640+2224	3.163	10.2	8.0	1.18	76	175.46	55.33	0.0008	0.3	[345 ]
J1643 $-$ 1224	4.622	9.7	8.4	4.86	159	147.02	25.07	0.000506	0.1	[189 , 320 ]
J1709+2313	4.631	10.3	8.1	1.83	89	22.7	15.3	0.0000187	0.3	[171 ]
J1713+0747	4.570	10.0	8.3	0.89	27	67.83	32.34	0.000075	0.3	[98 , 52 ]



J1732 $-$ 5049	5.313	9.8	8.43	1.81	?	5.26	3.98	0.0000098	0.2	[91 ]
J1745 $-$ 0952	19.376	9.5	9.1	2.38	?	4.94	2.38	0.0000180	0.1	[91 ]
J1751 $-$ 2857	3.915	9.7	8.3	1.40	?	110.75	32.53	0.000128	0.2	[294 ]
J1757 $-$ 5322	8.870	9.7	8.7	1.36	?	0.45	2.09	0.000004	0.6	[90 ]
B1800 $-$ 27	334.415	8.5	10.9	3.62	?	406.78	58.94	0.000507	0.1	[139 ]

J1804 $-$ 2717	9.343	9.5	8.8	1.17	?	11.13	7.28	0.000035	0.2	[187 ]
J1810 $-$ 2005	32.822	9.6	9.3	4.04	?	15.01	11.98	0.000025	0.3	[54 ]
B1831 $-$ 00	520.954	8.8	10.9	2.63	?	1.81	0.72	$> 0.0$	0.1	[87 ]
J1853+1303	4.092	9.9	8.3	1.60	?	115.65	40.8	0.0000237	0.3	[294 ]
B1855+09	5.362	9.7	8.5	1.00	29.2	12.33	9.23	0.000022	0.2	[279 , 155 ]

J1904+0412	71.095	10.1	9.4	4.01	?	14.93	9.63	0.00022	0.2	[54 ]
J1909 $-$ 3744	2.947	9.5	8.3	0.82	143	1.53	1.89	0.00000026	0.2	[133 ]

J1910+1256	4.984	9.9	8.3	1.90	?	58.47	21.1	0.0002302	0.2	[294 ]
J1911 $-$ 1114	3.626	0.0	0.0	1.59	183	2.72	1.76	$> 0.0$	0.1	[187 , 320 ]
J1918 $-$ 0642	7.646	$9 5.05× 10$	$8 4.33 × 10$	1.40	?	10.91	8.35	0.0000222		[91 ]

B1953+29	6.133	9.5	8.6	5.39	98	117.35	31.41	0.00033	0.2	[40 , 345 ]
B1957+20	1.607	9.4	8.1	1.53	190	0.38	0.09	$> 0.0$	0.02	[103 , 10 ]
J2016+1948	64.940	9.4	9.7	1.84	?	635.0	150.7	0.00128		[234 , 184 ]
J2019+2425	3.935	10.4	8.0	0.91	83	76.51	38.77	0.000111	0.3	[240 , 239 ]
J2033+1734	5.949	9.9	8.4	1.38	?	56.31	20.16	0.00013	0.2	[269 ]

J2051 $-$ 0827	4.509	9.7	8.4	1.28	14	0.10	0.05	$> 0.0$	0.03	[300 , 320 ]
J2129 $-$ 5721	3.726	9.5	8.4	2.55	56	6.63	3.50	$> 0.0$	0.1	[187 , 320 ]
J2145 $-$ 0750	16.052	10.3	8.6	0.50	38	6.84	10.16	0.000019	0.4	[22 , 320 ]
J2229+2643	2.978	10.4	7.9	1.43	113	93.02	18.91	0.00026	0.1	[345 ]
J2317+1439	3.445	10.6	7.9	1.89	68	2.46	2.31	$> 0.0$	0.2	[55 , 48 ]

Table 4:

Parameters for 50 low-eccentricity binary pulsars currently known in the Galactic disk. The parameters listed are defined in Tables 2 and 3.


PSR	$P$	$P$	Cluster	$Pb$	$x$	$e$	$m2$	Refs.
	[ms]	[ $× 10- 20$ ]		[days]	[s]		[ $M o .$ ]



J0023 $-$ 7204C	5.756	$- 4.98$	47 Tuc					[99 ]
J0024 $-$ 7204D	5.357	$- 0.34$	47 Tuc					[99 ]
J0024 $-$ 7205E	3.536	$+9.85$	47 Tuc	2.256	1.981	0.000315	0.15	[99 ]
J0024 $-$ 7204F	2.623	$+6.45$	47 Tuc					[99 ]
J0024 $-$ 7204G	4.040	$- 4.21$	47 Tuc					[99 ]

J0024 $-$ 7204H	3.210	$- 0.18$	47 Tuc	2.357	2.152	0.07056	0.16	[99 ]
J0024 $-$ 7204I	3.484	$- 4.58$	47 Tuc	0.229	0.038	$< 0.0004$	0.013	[99 ]
J0023 $-$ 7203J	2.100	$- 0.97$	47 Tuc	0.120	0.040	$< 0.00004$	0.021	[99 ]
J0024 $-$ 7204L	4.346	$- 12.2$	47 Tuc					[99 ]
J0023 $-$ 7205M	3.676	$- 3.84$	47 Tuc					[99 ]

J0024 $-$ 7204N	3.053	$- 2.18$	47 Tuc					[99 ]
J0024 $-$ 7204O	2.643	$+3.03$	47 Tuc	0.135	0.045	$< 0.00016$	0.022	[99 ]
P	3.643		47 Tuc	0.147	0.038		0.017	[53 ]
J0024 $-$ 7204Q	4.033	$+3.40$	47 Tuc	1.189	1.462	0.00008	0.17	[99 ]
R	3.480		47 Tuc	0.066	0.033		0.026	[99 ]

J0024 $-$ 7204S	2.830	$- 12.0$	47 Tuc	1.201	0.766	0.00039	0.088	[99 ]
J0024 $-$ 7204T	7.588	$+29.3$	47 Tuc	1.126	1.338	0.0004	0.16	[99 ]

J0024 $-$ 7203U	4.342	$+9.52$	47 Tuc	0.429	0.526	0.00014	0.12	[99 ]
V	4.810		47 Tuc	0.2	0.8		0.34	[53 ]
J0024 $-$ 7204W	2.352		47 Tuc	0.133	0.243		0.12	[99 ]

X	4.771		47 Tuc	?				[183 ]
Y	2.196		47 Tuc	0.521	0.671		0.13	[183 ]
J0514 $-$ 4002	4.990		NGC 1851	18.785	36	0.88	0.89	[100 ]
B1310+18A	33.163		M53	255	84	$< 0.01$	0.29	[166 ]
J1342+23A	2.545		M3	?				[265 ]



B	2.389		M3	1.42	1.9		0.20	[265 ]
C	2.166		M3	?				[265 ]
D	5.443		M3	?				[265 ]
B1516+02A	5.553	$+4.12$	M5					[6 ]
B1516+02B	7.946	$- 0.3$	M5	6.858	3.048	0.1378	0.11	[6 ]

C	2.484		M5	0.087	0.057		0.037	[265 ]
D	2.988		M5	1.22	1.6		0.19	[265 ]
E	3.182		M5	1.10	1.2		0.15	[265 ]
B1620 $-$ 26	11.075	$- 5.46$	M4	191.442	64.809	0.025315	0.27	[284 ]
B1639+36A	10.377	$< 4.5$	M13					[166 ]

B1639+36B	3.528		M13	1.259	1.38	$< 0.001$	0.15	[4 ]
C	3.722		M13					[265 ]

D	3.118		M13	0.591	0.92		0.17	[265 ]
E	2.487		M13	0.213	0.17		0.061	[265 ]
J1701 $-$ 3006A	5.241	$- 13.19$	NGC 6266	3.805	3.483	$< 0.000004$	0.19	[256 ]

J1701 $-$ 3006B	3.593	$- 34.97$	NGC 6266	0.144	0.252	$< 0.00007$	0.12	[256 ]
J1701 $-$ 3006C	3.806	$- 3.18$	NGC 6266	0.215	0.192	$< 0.00006$	0.069	[256 ]
D	3.418		NGC 6266	1.12	0.98		0.12	[63 ]
E	3.234		NGC 6266	0.16	0.07		0.030	[63 ]
F	2.295		NGC 6266	0.20	0.05		0.018	[63 ]

B1718 $-$ 19	1004	$+150000$	NGC 6342	0.258	0.352	$< 0.005$	0.11	[196 ]
J1740 $-$ 5340	3.650	$+16$	NGC 6397	1.354	1.652	$< 0.0001$	0.18	[79 ]
B1745 $-$ 20	288.60	$+40000$	NGC 6440					[203 ]
J1748 $-$ 2446A	11.563	$- 3.4$	Terzan 5	0.075	0.119	$< 0.0012$	0.087	[204 ]
J1748 $-$ 2446C	8.436	$- 60$	Terzan 5					[206 ]



D	4.713		Terzan 5					[262 ]
E	2.197		Terzan 5	60.06	23.6	$~ 0.02$	0.21	[266 ]
F	5.540		Terzan 5					[266 ]
G	21.671		Terzan 5					[266 ]
H	4.925		Terzan 5					[266 ]

I	9.570		Terzan 5	1.328	1.818	0.428	0.20	[266 ]
J	80.337		Terzan 5	1.102	2.454	0.350	0.33	[266 ]

K	2.969		Terzan 5					[266 ]
L	2.244		Terzan 5					[266 ]
M	3.569		Terzan 5	0.443	0.596		0.13	[266 ]

N	8.666		Terzan 5	0.385	1.619	0.000045	0.46	[266 ]
O	1.676		Terzan 5	0.259	0.112		0.035	[266 ]
P	1.728		Terzan 5	0.362	1.272		0.36	[266 ]
Q	2.812		Terzan 5	$> 1$ ?				[266 ]
R	5.028		Terzan 5					[266 ]

S	6.116		Terzan 5					[266 ]
T	7.084		Terzan 5					[266 ]
U	3.289		Terzan 5	$> 1$ ?				[266 ]
V	2.072		Terzan 5	0.503	0.567		0.11	[266 ]
W	4.205		Terzan 5	4.877	5.869	0.015	0.29	[266 ]



X	2.999		Terzan 5	$> 1$ ?				[266 ]
Y	2.048		Terzan 5	1.17	1.16		0.13	[266 ]
Z	2.462		Terzan 5	?	?			[233 ]
AA	5.788		Terzan 5	?	?			[233 ]
AB	5.12		Terzan 5	?	?			[233 ]
AC	5.09		Terzan 5	?	?			[233 ]
AD	1.40		Terzan 5	?	?			[233 ]

AE	3.66		Terzan 5	?	?			[233 ]
AF	3.30		Terzan 5	?	?			[233 ]
J1750 $-$ 37	111.61		NGC 6441	17.3	24.4	0.71	0.57	[255 ]

B1802 $-$ 07	23.100	$+47$	NGC 6539	2.616	3.920	0.212	0.29	[76 , 316 ]
J1803 $-$ 30	7.101		NGC 6522					[255 ]
J1807 $-$ 24A	3.059		NGC 6544	0.071	0.012		0.0089	[264 ]
B	4.186		NGC 6544	?				[63 ]
B1820 $-$ 30A	5.440	$+338$	NGC 6624					[35 ]

B1820 $-$ 30B	378.6	$+3150$	NGC 6624					[35 ]
C	405.9		NGC 6624					[63 ]
B1821 $-$ 24	3.054	$+161$	M28					[197 ]
J1905+01A	3.193		NGC 6749					[265 ]
B	4.968		NGC 6749					[265 ]

J1911 $-$ 5958A	3.266	$+0.30$	NGC 6752	0.837	1.206	$< 0.00001$	0.18	[78 ]
J1910 $-$ 5959B	8.357	$- 79$	NGC 6752					[78 ]
J1911 $-$ 6000C	5.277	$+0.2$	NGC 6752					[78 ]
J1910 $-$ 5959D	9.035	$+96$	NGC 6752					[78 ]
J1910 $-$ 5959E	4.571	$- 43$	NGC 6752					[78 ]



J1911+0102A	3.618	$- 0.65$	NGC 6760	0.140	0.037	$< 0.00013$	0.017	[101 ]
J1911+0101B	5.384	$- 0.2$	NGC 6760					[101 ]

J1953+18A	4.888		M71	0.176	0.078		0.032	[265 ]
B2127+11A	110.664	$- 2107$	M15					[4 ]
B2127+11B	56.133	$+956$	M15					[4 ]

B2127+11C	30.529	$+499$	M15	0.335	2.518	0.681	0.92	[4 ]
B2127+11D	4.802	$-107$	M15					[4 ]
B2127+11E	4.651	$+17$	M15					[4 ]
B2127+11F	4.027	$+3$	M15					[4 ]
B2127+11G	37.660	$+195$	M15					[4 ]

B2127+11H	6.743	$+2$	M15					[4 ]
J2140 $-$ 23A	11.019	$- 5.18$	M30	0.234		$< 0.00012$	0.10	[267 ]
B	13.0		M30	$> 0.1$		$> 0.52$		[267 ]

Table 5:

Parameters for the 108 pulsars currently known in globular clusters. In addition to the parameters defined in Tables 2 and 3, we also list the measured spin period derivative $P$ and name of associated cluster.