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) . |
B0031−07 | 77.00b | 1.26b | 0.942951403386(6) | 0.4070(4) | 4.79323268066(3) | 0.12 | 36.73(4) | 36.78(4) | 36.6243(6) |
B0136+57 | 319.0b | 2.65b | 0.272459130582(2) | 10.7010(2) | 11.30225636215(7) | 0.01 | 0.40368(1) | 0.40373(1) | 0.403268(5) |
B0148−06 | 261.0c | 4.60c | 1.46466489529(2) | 0.437(2) | 23.4309420922(4) | 0.53 | 53.1(2) | 53.4(2) | 52.469(6) |
B0154+61 | 383.7c | 1.80c | 2.35188677732(3) | 189.038(3) | 207.804907222(2) | 0.01 | 0.197256(3) | 0.197278(3) | 0.1973619(5) |
B0450+55 | 317.0b | 1.19b | 0.340731115855(1) | 2.39977(5) | 31.0821925829(1) | 0.13 | 2.25115(5) | 2.25407(5) | 2.27724(7) |
B0611+22 | 21.00c | 3.55c | 0.33500477221(4) | 59.05(4) | 0.044956192797(5) | 0 | 0.08995(7) | 0.08995(7) | 0.089332(2) |
B0626+24 | 84.00c | 3.00c | 0.476624376878(2) | 1.9944(2) | 1.210993642508(6) | 0.01 | 3.7890(4) | 3.7892(4) | 3.78649(6) |
B0727−18 | 179.9c | 2.04c | 0.510174601578(7) | 18.9659(6) | 8.7433773083(1) | 0 | 0.42649(1) | 0.42651(1) | 0.426675(4) |
B0809+74 | 102.0a | 0.43a | 1.292241576368(5) | 0.1679(3) | 33.7756638012(1) | 2.01 | 122.1(2) | 124.6(2) | 121.87(1) |
B0820+02 | 47.80c | 2.66c | 0.864872887877(9) | 0.1014(9) | 0.802517912658(8) | 0.08 | 135.2(12) | 135.3(12) | 131.157(8) |
B1530+27 | 144.0c | 1.60c | 1.12483633563(1) | 0.778(1) | 15.7478994453(2) | 0.2 | 22.93(4) | 22.98(4) | 22.877(2) |
B1540−06 | 247.4c | 3.11c | 0.709064757447(1) | 0.8793(1) | 15.07485676089(3) | 0.17 | 12.785(2) | 12.807(2) | 12.7818(6) |
B1541+09 | 277.0b | 7.20b | 0.74844877682(2) | 0.439(3) | 8.6162327085(2) | 0.2 | 27.02(17) | 27.07(17) | 27.438(3) |
B1642−03 | 386.4c | 3.97c | 0.387691475966(5) | 1.7791(2) | 15.7506425803(2) | 0.09 | 3.4550(4) | 3.4581(4) | 3.45241(3) |
B2154+40 | 264.0b | 3.40b | 1.52526824294(1) | 3.4342(7) | 33.7756301241(3) | 0.1 | 7.042(1) | 7.049(1) | 7.0452(1) |
B2351+61 | 268.0c | 2.42c | 0.944796588832(3) | 16.2657(3) | 30.2915037893(1) | 0.02 | 0.92094(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) . |
B0031−07 | 77.00b | 1.26b | 0.942951403386(6) | 0.4070(4) | 4.79323268066(3) | 0.12 | 36.73(4) | 36.78(4) | 36.6243(6) |
B0136+57 | 319.0b | 2.65b | 0.272459130582(2) | 10.7010(2) | 11.30225636215(7) | 0.01 | 0.40368(1) | 0.40373(1) | 0.403268(5) |
B0148−06 | 261.0c | 4.60c | 1.46466489529(2) | 0.437(2) | 23.4309420922(4) | 0.53 | 53.1(2) | 53.4(2) | 52.469(6) |
B0154+61 | 383.7c | 1.80c | 2.35188677732(3) | 189.038(3) | 207.804907222(2) | 0.01 | 0.197256(3) | 0.197278(3) | 0.1973619(5) |
B0450+55 | 317.0b | 1.19b | 0.340731115855(1) | 2.39977(5) | 31.0821925829(1) | 0.13 | 2.25115(5) | 2.25407(5) | 2.27724(7) |
B0611+22 | 21.00c | 3.55c | 0.33500477221(4) | 59.05(4) | 0.044956192797(5) | 0 | 0.08995(7) | 0.08995(7) | 0.089332(2) |
B0626+24 | 84.00c | 3.00c | 0.476624376878(2) | 1.9944(2) | 1.210993642508(6) | 0.01 | 3.7890(4) | 3.7892(4) | 3.78649(6) |
B0727−18 | 179.9c | 2.04c | 0.510174601578(7) | 18.9659(6) | 8.7433773083(1) | 0 | 0.42649(1) | 0.42651(1) | 0.426675(4) |
B0809+74 | 102.0a | 0.43a | 1.292241576368(5) | 0.1679(3) | 33.7756638012(1) | 2.01 | 122.1(2) | 124.6(2) | 121.87(1) |
B0820+02 | 47.80c | 2.66c | 0.864872887877(9) | 0.1014(9) | 0.802517912658(8) | 0.08 | 135.2(12) | 135.3(12) | 131.157(8) |
B1530+27 | 144.0c | 1.60c | 1.12483633563(1) | 0.778(1) | 15.7478994453(2) | 0.2 | 22.93(4) | 22.98(4) | 22.877(2) |
B1540−06 | 247.4c | 3.11c | 0.709064757447(1) | 0.8793(1) | 15.07485676089(3) | 0.17 | 12.785(2) | 12.807(2) | 12.7818(6) |
B1541+09 | 277.0b | 7.20b | 0.74844877682(2) | 0.439(3) | 8.6162327085(2) | 0.2 | 27.02(17) | 27.07(17) | 27.438(3) |
B1642−03 | 386.4c | 3.97c | 0.387691475966(5) | 1.7791(2) | 15.7506425803(2) | 0.09 | 3.4550(4) | 3.4581(4) | 3.45241(3) |
B2154+40 | 264.0b | 3.40b | 1.52526824294(1) | 3.4342(7) | 33.7756301241(3) | 0.1 | 7.042(1) | 7.049(1) | 7.0452(1) |
B2351+61 | 268.0c | 2.42c | 0.944796588832(3) | 16.2657(3) | 30.2915037893(1) | 0.02 | 0.92094(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).
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) . |
B0031−07 | 77.00b | 1.26b | 0.942951403386(6) | 0.4070(4) | 4.79323268066(3) | 0.12 | 36.73(4) | 36.78(4) | 36.6243(6) |
B0136+57 | 319.0b | 2.65b | 0.272459130582(2) | 10.7010(2) | 11.30225636215(7) | 0.01 | 0.40368(1) | 0.40373(1) | 0.403268(5) |
B0148−06 | 261.0c | 4.60c | 1.46466489529(2) | 0.437(2) | 23.4309420922(4) | 0.53 | 53.1(2) | 53.4(2) | 52.469(6) |
B0154+61 | 383.7c | 1.80c | 2.35188677732(3) | 189.038(3) | 207.804907222(2) | 0.01 | 0.197256(3) | 0.197278(3) | 0.1973619(5) |
B0450+55 | 317.0b | 1.19b | 0.340731115855(1) | 2.39977(5) | 31.0821925829(1) | 0.13 | 2.25115(5) | 2.25407(5) | 2.27724(7) |
B0611+22 | 21.00c | 3.55c | 0.33500477221(4) | 59.05(4) | 0.044956192797(5) | 0 | 0.08995(7) | 0.08995(7) | 0.089332(2) |
B0626+24 | 84.00c | 3.00c | 0.476624376878(2) | 1.9944(2) | 1.210993642508(6) | 0.01 | 3.7890(4) | 3.7892(4) | 3.78649(6) |
B0727−18 | 179.9c | 2.04c | 0.510174601578(7) | 18.9659(6) | 8.7433773083(1) | 0 | 0.42649(1) | 0.42651(1) | 0.426675(4) |
B0809+74 | 102.0a | 0.43a | 1.292241576368(5) | 0.1679(3) | 33.7756638012(1) | 2.01 | 122.1(2) | 124.6(2) | 121.87(1) |
B0820+02 | 47.80c | 2.66c | 0.864872887877(9) | 0.1014(9) | 0.802517912658(8) | 0.08 | 135.2(12) | 135.3(12) | 131.157(8) |
B1530+27 | 144.0c | 1.60c | 1.12483633563(1) | 0.778(1) | 15.7478994453(2) | 0.2 | 22.93(4) | 22.98(4) | 22.877(2) |
B1540−06 | 247.4c | 3.11c | 0.709064757447(1) | 0.8793(1) | 15.07485676089(3) | 0.17 | 12.785(2) | 12.807(2) | 12.7818(6) |
B1541+09 | 277.0b | 7.20b | 0.74844877682(2) | 0.439(3) | 8.6162327085(2) | 0.2 | 27.02(17) | 27.07(17) | 27.438(3) |
B1642−03 | 386.4c | 3.97c | 0.387691475966(5) | 1.7791(2) | 15.7506425803(2) | 0.09 | 3.4550(4) | 3.4581(4) | 3.45241(3) |
B2154+40 | 264.0b | 3.40b | 1.52526824294(1) | 3.4342(7) | 33.7756301241(3) | 0.1 | 7.042(1) | 7.049(1) | 7.0452(1) |
B2351+61 | 268.0c | 2.42c | 0.944796588832(3) | 16.2657(3) | 30.2915037893(1) | 0.02 | 0.92094(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) . |
B0031−07 | 77.00b | 1.26b | 0.942951403386(6) | 0.4070(4) | 4.79323268066(3) | 0.12 | 36.73(4) | 36.78(4) | 36.6243(6) |
B0136+57 | 319.0b | 2.65b | 0.272459130582(2) | 10.7010(2) | 11.30225636215(7) | 0.01 | 0.40368(1) | 0.40373(1) | 0.403268(5) |
B0148−06 | 261.0c | 4.60c | 1.46466489529(2) | 0.437(2) | 23.4309420922(4) | 0.53 | 53.1(2) | 53.4(2) | 52.469(6) |
B0154+61 | 383.7c | 1.80c | 2.35188677732(3) | 189.038(3) | 207.804907222(2) | 0.01 | 0.197256(3) | 0.197278(3) | 0.1973619(5) |
B0450+55 | 317.0b | 1.19b | 0.340731115855(1) | 2.39977(5) | 31.0821925829(1) | 0.13 | 2.25115(5) | 2.25407(5) | 2.27724(7) |
B0611+22 | 21.00c | 3.55c | 0.33500477221(4) | 59.05(4) | 0.044956192797(5) | 0 | 0.08995(7) | 0.08995(7) | 0.089332(2) |
B0626+24 | 84.00c | 3.00c | 0.476624376878(2) | 1.9944(2) | 1.210993642508(6) | 0.01 | 3.7890(4) | 3.7892(4) | 3.78649(6) |
B0727−18 | 179.9c | 2.04c | 0.510174601578(7) | 18.9659(6) | 8.7433773083(1) | 0 | 0.42649(1) | 0.42651(1) | 0.426675(4) |
B0809+74 | 102.0a | 0.43a | 1.292241576368(5) | 0.1679(3) | 33.7756638012(1) | 2.01 | 122.1(2) | 124.6(2) | 121.87(1) |
B0820+02 | 47.80c | 2.66c | 0.864872887877(9) | 0.1014(9) | 0.802517912658(8) | 0.08 | 135.2(12) | 135.3(12) | 131.157(8) |
B1530+27 | 144.0c | 1.60c | 1.12483633563(1) | 0.778(1) | 15.7478994453(2) | 0.2 | 22.93(4) | 22.98(4) | 22.877(2) |
B1540−06 | 247.4c | 3.11c | 0.709064757447(1) | 0.8793(1) | 15.07485676089(3) | 0.17 | 12.785(2) | 12.807(2) | 12.7818(6) |
B1541+09 | 277.0b | 7.20b | 0.74844877682(2) | 0.439(3) | 8.6162327085(2) | 0.2 | 27.02(17) | 27.07(17) | 27.438(3) |
B1642−03 | 386.4c | 3.97c | 0.387691475966(5) | 1.7791(2) | 15.7506425803(2) | 0.09 | 3.4550(4) | 3.4581(4) | 3.45241(3) |
B2154+40 | 264.0b | 3.40b | 1.52526824294(1) | 3.4342(7) | 33.7756301241(3) | 0.1 | 7.042(1) | 7.049(1) | 7.0452(1) |
B2351+61 | 268.0c | 2.42c | 0.944796588832(3) | 16.2657(3) | 30.2915037893(1) | 0.02 | 0.92094(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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