Table 4.

Parameters relative to the Shklovsky effect and newly calculated characteristic ages of 16 pulsars.

|$V_{\rm T}{}^{*}$|d*P|$\dot{P}_{\rm m}$||$\dot{P}_{\rm s}$||$\dot{P}_{\rm s}/\dot{P}_{\rm m}$|τm|$\tau _{\rm i}{}^{\dagger }$||$\tau _{\rm p}{}^{\dagger }$|
Name(km s−1)(kpc)(s)(10−15 s s−1)(10−19 s s−1)(%)(Myr)(Myr)(Myr)
B0031−0777.00b1.26b0.942951403386(6)0.4070(4)4.79323268066(3)0.1236.73(4)36.78(4)36.6243(6)
B0136+57319.0b2.65b0.272459130582(2)10.7010(2)11.30225636215(7)0.010.40368(1)0.40373(1)0.403268(5)
B0148−06261.0c4.60c1.46466489529(2)0.437(2)23.4309420922(4)0.5353.1(2)53.4(2)52.469(6)
B0154+61383.7c1.80c2.35188677732(3)189.038(3)207.804907222(2)0.010.197256(3)0.197278(3)0.1973619(5)
B0450+55317.0b1.19b0.340731115855(1)2.39977(5)31.0821925829(1)0.132.25115(5)2.25407(5)2.27724(7)
B0611+2221.00c3.55c0.33500477221(4)59.05(4)0.044956192797(5)00.08995(7)0.08995(7)0.089332(2)
B0626+2484.00c3.00c0.476624376878(2)1.9944(2)1.210993642508(6)0.013.7890(4)3.7892(4)3.78649(6)
B0727−18179.9c2.04c0.510174601578(7)18.9659(6)8.7433773083(1)00.42649(1)0.42651(1)0.426675(4)
B0809+74102.0a0.43a1.292241576368(5)0.1679(3)33.7756638012(1)2.01122.1(2)124.6(2)121.87(1)
B0820+0247.80c2.66c0.864872887877(9)0.1014(9)0.802517912658(8)0.08135.2(12)135.3(12)131.157(8)
B1530+27144.0c1.60c1.12483633563(1)0.778(1)15.7478994453(2)0.222.93(4)22.98(4)22.877(2)
B1540−06247.4c3.11c0.709064757447(1)0.8793(1)15.07485676089(3)0.1712.785(2)12.807(2)12.7818(6)
B1541+09277.0b7.20b0.74844877682(2)0.439(3)8.6162327085(2)0.227.02(17)27.07(17)27.438(3)
B1642−03386.4c3.97c0.387691475966(5)1.7791(2)15.7506425803(2)0.093.4550(4)3.4581(4)3.45241(3)
B2154+40264.0b3.40b1.52526824294(1)3.4342(7)33.7756301241(3)0.17.042(1)7.049(1)7.0452(1)
B2351+61268.0c2.42c0.944796588832(3)16.2657(3)30.2915037893(1)0.020.92094(2)0.92111(2)0.921087(5)
|$V_{\rm T}{}^{*}$|d*P|$\dot{P}_{\rm m}$||$\dot{P}_{\rm s}$||$\dot{P}_{\rm s}/\dot{P}_{\rm m}$|τm|$\tau _{\rm i}{}^{\dagger }$||$\tau _{\rm p}{}^{\dagger }$|
Name(km s−1)(kpc)(s)(10−15 s s−1)(10−19 s s−1)(%)(Myr)(Myr)(Myr)
B0031−0777.00b1.26b0.942951403386(6)0.4070(4)4.79323268066(3)0.1236.73(4)36.78(4)36.6243(6)
B0136+57319.0b2.65b0.272459130582(2)10.7010(2)11.30225636215(7)0.010.40368(1)0.40373(1)0.403268(5)
B0148−06261.0c4.60c1.46466489529(2)0.437(2)23.4309420922(4)0.5353.1(2)53.4(2)52.469(6)
B0154+61383.7c1.80c2.35188677732(3)189.038(3)207.804907222(2)0.010.197256(3)0.197278(3)0.1973619(5)
B0450+55317.0b1.19b0.340731115855(1)2.39977(5)31.0821925829(1)0.132.25115(5)2.25407(5)2.27724(7)
B0611+2221.00c3.55c0.33500477221(4)59.05(4)0.044956192797(5)00.08995(7)0.08995(7)0.089332(2)
B0626+2484.00c3.00c0.476624376878(2)1.9944(2)1.210993642508(6)0.013.7890(4)3.7892(4)3.78649(6)
B0727−18179.9c2.04c0.510174601578(7)18.9659(6)8.7433773083(1)00.42649(1)0.42651(1)0.426675(4)
B0809+74102.0a0.43a1.292241576368(5)0.1679(3)33.7756638012(1)2.01122.1(2)124.6(2)121.87(1)
B0820+0247.80c2.66c0.864872887877(9)0.1014(9)0.802517912658(8)0.08135.2(12)135.3(12)131.157(8)
B1530+27144.0c1.60c1.12483633563(1)0.778(1)15.7478994453(2)0.222.93(4)22.98(4)22.877(2)
B1540−06247.4c3.11c0.709064757447(1)0.8793(1)15.07485676089(3)0.1712.785(2)12.807(2)12.7818(6)
B1541+09277.0b7.20b0.74844877682(2)0.439(3)8.6162327085(2)0.227.02(17)27.07(17)27.438(3)
B1642−03386.4c3.97c0.387691475966(5)1.7791(2)15.7506425803(2)0.093.4550(4)3.4581(4)3.45241(3)
B2154+40264.0b3.40b1.52526824294(1)3.4342(7)33.7756301241(3)0.17.042(1)7.049(1)7.0452(1)
B2351+61268.0c2.42c0.944796588832(3)16.2657(3)30.2915037893(1)0.020.92094(2)0.92111(2)0.921087(5)

*References: a. Brisken et al. (2002); b. Chatterjee et al. (2009); c. Deller et al. (2019).

τi is the intrinsic age with the Shklovsky effect subtracted. τp is calculated based on previous rotation solutions in Hobbs et al. (2004).

Table 4.

Parameters relative to the Shklovsky effect and newly calculated characteristic ages of 16 pulsars.

|$V_{\rm T}{}^{*}$|d*P|$\dot{P}_{\rm m}$||$\dot{P}_{\rm s}$||$\dot{P}_{\rm s}/\dot{P}_{\rm m}$|τm|$\tau _{\rm i}{}^{\dagger }$||$\tau _{\rm p}{}^{\dagger }$|
Name(km s−1)(kpc)(s)(10−15 s s−1)(10−19 s s−1)(%)(Myr)(Myr)(Myr)
B0031−0777.00b1.26b0.942951403386(6)0.4070(4)4.79323268066(3)0.1236.73(4)36.78(4)36.6243(6)
B0136+57319.0b2.65b0.272459130582(2)10.7010(2)11.30225636215(7)0.010.40368(1)0.40373(1)0.403268(5)
B0148−06261.0c4.60c1.46466489529(2)0.437(2)23.4309420922(4)0.5353.1(2)53.4(2)52.469(6)
B0154+61383.7c1.80c2.35188677732(3)189.038(3)207.804907222(2)0.010.197256(3)0.197278(3)0.1973619(5)
B0450+55317.0b1.19b0.340731115855(1)2.39977(5)31.0821925829(1)0.132.25115(5)2.25407(5)2.27724(7)
B0611+2221.00c3.55c0.33500477221(4)59.05(4)0.044956192797(5)00.08995(7)0.08995(7)0.089332(2)
B0626+2484.00c3.00c0.476624376878(2)1.9944(2)1.210993642508(6)0.013.7890(4)3.7892(4)3.78649(6)
B0727−18179.9c2.04c0.510174601578(7)18.9659(6)8.7433773083(1)00.42649(1)0.42651(1)0.426675(4)
B0809+74102.0a0.43a1.292241576368(5)0.1679(3)33.7756638012(1)2.01122.1(2)124.6(2)121.87(1)
B0820+0247.80c2.66c0.864872887877(9)0.1014(9)0.802517912658(8)0.08135.2(12)135.3(12)131.157(8)
B1530+27144.0c1.60c1.12483633563(1)0.778(1)15.7478994453(2)0.222.93(4)22.98(4)22.877(2)
B1540−06247.4c3.11c0.709064757447(1)0.8793(1)15.07485676089(3)0.1712.785(2)12.807(2)12.7818(6)
B1541+09277.0b7.20b0.74844877682(2)0.439(3)8.6162327085(2)0.227.02(17)27.07(17)27.438(3)
B1642−03386.4c3.97c0.387691475966(5)1.7791(2)15.7506425803(2)0.093.4550(4)3.4581(4)3.45241(3)
B2154+40264.0b3.40b1.52526824294(1)3.4342(7)33.7756301241(3)0.17.042(1)7.049(1)7.0452(1)
B2351+61268.0c2.42c0.944796588832(3)16.2657(3)30.2915037893(1)0.020.92094(2)0.92111(2)0.921087(5)
|$V_{\rm T}{}^{*}$|d*P|$\dot{P}_{\rm m}$||$\dot{P}_{\rm s}$||$\dot{P}_{\rm s}/\dot{P}_{\rm m}$|τm|$\tau _{\rm i}{}^{\dagger }$||$\tau _{\rm p}{}^{\dagger }$|
Name(km s−1)(kpc)(s)(10−15 s s−1)(10−19 s s−1)(%)(Myr)(Myr)(Myr)
B0031−0777.00b1.26b0.942951403386(6)0.4070(4)4.79323268066(3)0.1236.73(4)36.78(4)36.6243(6)
B0136+57319.0b2.65b0.272459130582(2)10.7010(2)11.30225636215(7)0.010.40368(1)0.40373(1)0.403268(5)
B0148−06261.0c4.60c1.46466489529(2)0.437(2)23.4309420922(4)0.5353.1(2)53.4(2)52.469(6)
B0154+61383.7c1.80c2.35188677732(3)189.038(3)207.804907222(2)0.010.197256(3)0.197278(3)0.1973619(5)
B0450+55317.0b1.19b0.340731115855(1)2.39977(5)31.0821925829(1)0.132.25115(5)2.25407(5)2.27724(7)
B0611+2221.00c3.55c0.33500477221(4)59.05(4)0.044956192797(5)00.08995(7)0.08995(7)0.089332(2)
B0626+2484.00c3.00c0.476624376878(2)1.9944(2)1.210993642508(6)0.013.7890(4)3.7892(4)3.78649(6)
B0727−18179.9c2.04c0.510174601578(7)18.9659(6)8.7433773083(1)00.42649(1)0.42651(1)0.426675(4)
B0809+74102.0a0.43a1.292241576368(5)0.1679(3)33.7756638012(1)2.01122.1(2)124.6(2)121.87(1)
B0820+0247.80c2.66c0.864872887877(9)0.1014(9)0.802517912658(8)0.08135.2(12)135.3(12)131.157(8)
B1530+27144.0c1.60c1.12483633563(1)0.778(1)15.7478994453(2)0.222.93(4)22.98(4)22.877(2)
B1540−06247.4c3.11c0.709064757447(1)0.8793(1)15.07485676089(3)0.1712.785(2)12.807(2)12.7818(6)
B1541+09277.0b7.20b0.74844877682(2)0.439(3)8.6162327085(2)0.227.02(17)27.07(17)27.438(3)
B1642−03386.4c3.97c0.387691475966(5)1.7791(2)15.7506425803(2)0.093.4550(4)3.4581(4)3.45241(3)
B2154+40264.0b3.40b1.52526824294(1)3.4342(7)33.7756301241(3)0.17.042(1)7.049(1)7.0452(1)
B2351+61268.0c2.42c0.944796588832(3)16.2657(3)30.2915037893(1)0.020.92094(2)0.92111(2)0.921087(5)

*References: a. Brisken et al. (2002); b. Chatterjee et al. (2009); c. Deller et al. (2019).

τi is the intrinsic age with the Shklovsky effect subtracted. τp is calculated based on previous rotation solutions in Hobbs et al. (2004).

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