Table 1.
J1513 and J2017 parameters obtained from Sanpa-arsa (2016), the ATNF catalogue, and the Third Fermi Large Area Telescope catalogue of γ-ray pulsars (Smith et al. 2023).
MSP | J2017 | J1513 |
---|---|---|
RA α (J2000) | 20h17m46.s1478(8) | 15h13m23.s32059(6) |
Dec δ (J2000) | −16 ° 14′15.″51(5) | −25 ° 50′31.″285(3) |
Galactic longitude l, deg | 27.314 | 338.820 |
Galactic latitude b, deg | −26.220 | 26.964 |
Spin period P, ms | 2.3142872649224(4) | 2.1190675651177(1) |
Period derivative , s s−1 | 2.45(5) × 10−21 | 21.61(2) × 10−21 |
Orbital period Pb, d | 0.0978252578(4) | 0.1786354505(8) |
Projected semi-major axis x, lt-s | 0.043655(5) | 0.0408132(7) |
Epoch of ascending node Tasc, MJD | 56704.756314(2) | 56728.4539340(6) |
Mass function fM, M⊙ | 9.334(3) × 10−6 | 2.2874(1) × 10−6 |
Dispersion measure DM, pc cm−3 | 25.4380(4) | 46.86(7) |
Distance DYMW16, kpc | 1.4 | 4.0 |
Distance DNE2001, kpc | 1.1 | 2.0 |
Characteristic age , Gyr | 15 | 1.55 |
Spin-down luminosity , erg s−1 | 7.8 × 1033 | 9.0 × 1034 |
Minimum companion mass Mc, min, M⊙ | 0.03 | 0.02 |
p.m. in RA direction μαcos δ, mas yr−1 | – | −6.3(1) |
p.m. in Dec direction μδ, mas yr−1 | – | −3.5(4) |
Notes. Numbers in parentheses denote 1σ uncertainties relating to the last significant digit.
DYMW16 and DNE2001 are dispersion measure distances derived using the YMW16 (Yao et al. 2017) and NE2001 (Cordes & Lazio 2002) models for the distribution of free electrons in the Galaxy, respectively. The minimum companion mass was calculated for the pulsar mass of Mp = 1.4 M⊙ and orbital inclination of i = 90°. p.m. = proper motion.
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