Optical spectral observations of three binary millisecond pulsars
arXiv:2307.02167 · doi:10.1093/mnras/stad2021
Abstract
We present the results of optical spectroscopy of stellar companions to three binary millisecond pulsars, PSRs J06212514, J23171439 and J23024442, obtained with the Gran Telescopio Canarias. The spectrum of the J06212514 companion shows a blue continuum and prominent Balmer absorption lines. The latter are also resolved in the spectrum of the J23171439 companion, showing that both are DA-type white dwarfs. No spectral features are detected for the J23024442 companion, however, its broadband magnitudes and the spectral shape of the continuum emission imply that this is also a DA-type white dwarf. Based on the spectral analyses, we conclude that the companions of J06212514 and J23171439 are relatively hot, with effective temperatures 8600200 and 96002000~K, respectively, while the J23024442 companion is significantly cooler, 6000~K. We also estimated the distance to J06212514 of 1.10.3 kpc and argue that its companion and the companion of J23171439 are He-core white dwarfs providing constraints on their cooling ages of 2 Gyr.
arXiv comment9 pages, 8 figures. Paper accepted to MNRAS
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