A GTC spectroscopic study of three spider pulsar companions: line-based temperatures, a new face-on redback, and improved mass constraints

TL;DR

This study uses phase-resolved spectroscopy of three spider pulsar companions to measure temperatures, radial velocities, and masses, revealing system geometries, asymmetric heating, and metal enrichment, with implications for neutron star mass constraints.

Contribution

First spectroscopic measurements of three spider pulsar companions, providing new mass constraints, temperature profiles, and insights into system geometries and heating effects.

Findings

Radial velocity semi-amplitudes vary with absorption features used.

Mass constraints for two systems, revealing high neutron star masses.

Evidence of asymmetric heating and metal enrichment in companions.

Abstract

We present GTC-OSIRIS phase-resolved optical spectroscopy of three compact binary MSPs, or 'spiders': PSR J1048+2339, PSR J1810+1744, and (for the first time) PSR J1908+2105. For the companion in each system, the temperature is traced throughout its orbit, and radial velocities are measured. The radial velocities are found to vary with the absorption features used when measuring them, resulting in different radial velocity curve semi-amplitudes: for J1048 ($K_\mathrm{metals, red} = 344 \pm 4$ km s$^{-1}$, $K_\mathrm{metals, blue} = 372 \pm 3$ km s$^{-1}$) and, tentatively, for J1810 ($K_\mathrm{Balmer} = 448 \pm 19$ km s$^{-1}$, $K_\mathrm{metals} = 491 \pm 32$ km s$^{-1}$). With existing inclination constraints, this gives the neutron star (NS) and companion masses $M_\mathrm{NS} = 1.50 - 2.04$ $M_\odot$ and $M_2 = 0.32 - 0.40$ $M_\odot$ for J1048, and $M_\mathrm{NS} > 1.7$ $M_\odot$ and $M_2 = 0.05 - 0.08$ $M_\odot$ for J1810. For J1908, we find an upper limit of $K_2 < 32$ km s$^{-1}$, which constrains its mass ratio $q = M_2 / M_\mathrm{NS} > 0.55$ and inclination $i < 6.0^\circ$, revealing the previously misunderstood system to be the highest mass ratio, lowest inclination redback yet. This raises questions for the origins of its substantial radio eclipses. Additionally, we find evidence of asymmetric heating in J1048 and J1810, and signs of metal enrichment in J1908. We also explore the impact of inclination on spectroscopic temperatures, and demonstrate that the temperature measured at quadrature ($\phi = 0.25, 0.75$) is essentially independent of inclination, and thus can provide additional constraints on photometric modelling.