TY - JOUR
T1 - Hubble Space Telescope Nondetection of PSR J2144-3933
T2 - The Coldest Known Neutron Star
AU - Guillot, Sebastien
AU - Pavlov, George G.
AU - Reyes, Cristobal
AU - Reisenegger, Andreas
AU - Rodriguez, Luis E.
AU - Rangelov, Blagoy
AU - Kargaltsev, Oleg
N1 - Publisher Copyright:
© 2019. The American Astronomical Society. All rights reserved.
PY - 2019/4/1
Y1 - 2019/4/1
N2 - We report nondetections of the ∼3 ×10 8 yr old, slow, isolated, rotation-powered pulsar PSR J2144-3933 in observations with the Hubble Space Telescope in one optical band (F475X) and two far-ultraviolet bands (F125LP and F140LP), yielding upper bounds F F475X < 22.7 nJy, F F125LP < 5.9 nJy, and F F140LP < 19.5 nJy and at the pivot wavelengths 4940 Å, 1438 Å and 1528 Å, respectively. Assuming a blackbody spectrum, we deduce a conservative upper bound on the surface (unredshifted) temperature of the pulsar of 42,000 K. This makes PSR J2144-3933 the coldest known neutron star, allowing us to study thermal evolution models of old neutron stars. This temperature is consistent with models with either direct or modified Urca reactions including rotochemical heating, and, considering frictional heating from the motion of neutron vortex lines, it puts an upper bound on the excess angular momentum in the neutron superfluid, J < 10 44 erg s.
AB - We report nondetections of the ∼3 ×10 8 yr old, slow, isolated, rotation-powered pulsar PSR J2144-3933 in observations with the Hubble Space Telescope in one optical band (F475X) and two far-ultraviolet bands (F125LP and F140LP), yielding upper bounds F F475X < 22.7 nJy, F F125LP < 5.9 nJy, and F F140LP < 19.5 nJy and at the pivot wavelengths 4940 Å, 1438 Å and 1528 Å, respectively. Assuming a blackbody spectrum, we deduce a conservative upper bound on the surface (unredshifted) temperature of the pulsar of 42,000 K. This makes PSR J2144-3933 the coldest known neutron star, allowing us to study thermal evolution models of old neutron stars. This temperature is consistent with models with either direct or modified Urca reactions including rotochemical heating, and, considering frictional heating from the motion of neutron vortex lines, it puts an upper bound on the excess angular momentum in the neutron superfluid, J < 10 44 erg s.
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U2 - 10.3847/1538-4357/ab0f38
DO - 10.3847/1538-4357/ab0f38
M3 - Article
AN - SCOPUS:85064440754
SN - 0004-637X
VL - 874
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 2
M1 - 175
ER -