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M. C. Miller
209. T.E. Strohmayer, A.L. Watts, The 2004 hyperflare from SGR 1806-20: further evidence
for global torsional vibrations. Astrophys. J. 653, 593–601 (2006). https://doi.org/10.1086/
508703
210. V. Suleimanov, J. Poutanen, M. Revnivtsev, K. Werner, A neutron star stiff equation of state
derived from cooling phases of the X-ray burster 4U 1724-307. Astrophys. J. 742, 122 (2011).
https://doi.org/10.1088/0004-637X/742/2/122
211. V. Suleimanov, J. Poutanen, K. Werner, X-ray bursting neutron star atmosphere models using
an exact relativistic kinetic equation for Compton scattering. Astron. Astrophys. 545, A120
(2012). https://doi.org/10.1051/0004-6361/201219480
212. R.E. Taam, R.E. Picklum, Nuclear fusion and carbon flashes on neutron stars. Astrophys. J.
224, 210–216 (1978). https://doi.org/10.1086/156367
213. R.E. Taam, S.E. Woosley, T.A. Weaver, D.Q. Lamb, Successive X-ray bursts from accreting
neutron stars. Astrophys. J. 413, 324–332 (1993). https://doi.org/10.1086/173000
214. N.R. Tanvir, A.J. Levan, A.S. Fruchter, J. Hjorth, R.A. Hounsell, K. Wiersema, R.L.
Tunnicliffe, A ‘kilonova’ associated with the short-duration γ -ray burst GRB130603B.
Nature 500, 547–549 (2013). https://doi.org/10.1038/nature12505
215. J.A. Tomsick, M.W. Muterspaugh, Masses of neutron stars in high-mass X-ray binaries with
optical astrometry. Astrophys. J. 719, 958–965 (2010). https://doi.org/10.1088/0004-637X/
719/1/958
216. M. Troyer, U.-J. Wiese, Computational complexity and fundamental limitations to fermionic
Quantum Monte Carlo simulations. Phys. Rev. Lett. 94(17), 170201–+ (2005). https://doi.org/
10.1103/PhysRevLett.94.170201
217. G. Ushomirsky, R.E. Rutledge, Time-variable emission from transiently accreting neutron
stars in quiescence due to deep crustal heating. Mon. Not. R. Astron. Soc. 325, 1157–1166
(2001). https://doi.org/10.1046/j.1365-8711.2001.04515.x
218. G. Ushomirsky, C. Cutler, L. Bildsten, Deformations of accreting neutron star crusts and
gravitational wave emission. Mon. Not. R. Astron. Soc. 319, 902–932 (2000). https://doi.org/
10.1046/j.1365-8711.2000.03938.x
219. C. Van Den Broeck, Astrophysics, cosmology, and fundamental physics with compact binary
coalescence and the Einstein Telescope. J. Phys. Conf. Ser. 484(1), 012008 (2014). https://
doi.org/10.1088/1742-6596/484/1/012008
220. M. van der Sluys, I. Mandel, V. Raymond, V. Kalogera, C. Röver, N. Christensen, Parameter
estimation for signals from compact binary inspirals injected into LIGO data. Classical
Quantum Gravity 26(20), 204010 (2009). https://doi.org/10.1088/0264-9381/26/20/204010
221. C.A. van Eysden, A. Melatos, Gravitational radiation from pulsar glitches. Classical Quantum
Gravity 25(22), 225020–+ (2008). https://doi.org/10.1088/0264-9381/25/22/225020
222. M.H. van Kerkwijk, D.L. Kaplan, Isolated neutron stars: magnetic fields, distances,and
spectra. Astrophys. Space Sci. 308, 191–201 (2007). https://doi.org/10.1007/s10509-0079343-9
223. M.H. van Kerkwijk, R.P. Breton, S.R. Kulkarni, Evidence for a massive neutron star from a
radial-velocity study of the companion to the black-widow pulsar PSR B1957+20. Astrophys.
J. 728, 95 (2011). https://doi.org/10.1088/0004-637X/728/2/95
224. J. van Paradijs, Possible observational constraints on the mass-radius relation of neutron stars.
Astrophys. J. 234, 609–611 (1979). https://doi.org/10.1086/157535
225. T. Venumadhav, A. Zimmerman, C.M. Hirata, The stability of tidally deformed neutron stars
to three- and four-mode coupling. Astrophys. J. 781, 23 (2014). https://doi.org/10.1088/0004637X/781/1/23
226. K. Viironen, J. Poutanen, Light curves and polarization of accretion- and nuclear-powered
millisecond pulsars. Astron. Astrophys. 426, 985–997 (2004). https://doi.org/10.1051/00046361:20041084
227. A.R. Villarreal, T.E. Strohmayer, Discovery of the neutron star spin frequency in EXO 0748676. Astrophys. J. Lett. 614, L121–L124 (2004). https://doi.org/10.1086/425737
228. F.M. Walter, J.M. Lattimer, A revised parallax and its implications for RX J185635-3754.
Astrophys. J. Lett. 576, L145–L148 (2002). https://doi.org/10.1086/343850
M. C. Miller
209. T.E. Strohmayer, A.L. Watts, The 2004 hyperflare from SGR 1806-20: further evidence
for global torsional vibrations. Astrophys. J. 653, 593–601 (2006). https://doi.org/10.1086/
508703
210. V. Suleimanov, J. Poutanen, M. Revnivtsev, K. Werner, A neutron star stiff equation of state
derived from cooling phases of the X-ray burster 4U 1724-307. Astrophys. J. 742, 122 (2011).
https://doi.org/10.1088/0004-637X/742/2/122
211. V. Suleimanov, J. Poutanen, K. Werner, X-ray bursting neutron star atmosphere models using
an exact relativistic kinetic equation for Compton scattering. Astron. Astrophys. 545, A120
(2012). https://doi.org/10.1051/0004-6361/201219480
212. R.E. Taam, R.E. Picklum, Nuclear fusion and carbon flashes on neutron stars. Astrophys. J.
224, 210–216 (1978). https://doi.org/10.1086/156367
213. R.E. Taam, S.E. Woosley, T.A. Weaver, D.Q. Lamb, Successive X-ray bursts from accreting
neutron stars. Astrophys. J. 413, 324–332 (1993). https://doi.org/10.1086/173000
214. N.R. Tanvir, A.J. Levan, A.S. Fruchter, J. Hjorth, R.A. Hounsell, K. Wiersema, R.L.
Tunnicliffe, A ‘kilonova’ associated with the short-duration γ -ray burst GRB130603B.
Nature 500, 547–549 (2013). https://doi.org/10.1038/nature12505
215. J.A. Tomsick, M.W. Muterspaugh, Masses of neutron stars in high-mass X-ray binaries with
optical astrometry. Astrophys. J. 719, 958–965 (2010). https://doi.org/10.1088/0004-637X/
719/1/958
216. M. Troyer, U.-J. Wiese, Computational complexity and fundamental limitations to fermionic
Quantum Monte Carlo simulations. Phys. Rev. Lett. 94(17), 170201–+ (2005). https://doi.org/
10.1103/PhysRevLett.94.170201
217. G. Ushomirsky, R.E. Rutledge, Time-variable emission from transiently accreting neutron
stars in quiescence due to deep crustal heating. Mon. Not. R. Astron. Soc. 325, 1157–1166
(2001). https://doi.org/10.1046/j.1365-8711.2001.04515.x
218. G. Ushomirsky, C. Cutler, L. Bildsten, Deformations of accreting neutron star crusts and
gravitational wave emission. Mon. Not. R. Astron. Soc. 319, 902–932 (2000). https://doi.org/
10.1046/j.1365-8711.2000.03938.x
219. C. Van Den Broeck, Astrophysics, cosmology, and fundamental physics with compact binary
coalescence and the Einstein Telescope. J. Phys. Conf. Ser. 484(1), 012008 (2014). https://
doi.org/10.1088/1742-6596/484/1/012008
220. M. van der Sluys, I. Mandel, V. Raymond, V. Kalogera, C. Röver, N. Christensen, Parameter
estimation for signals from compact binary inspirals injected into LIGO data. Classical
Quantum Gravity 26(20), 204010 (2009). https://doi.org/10.1088/0264-9381/26/20/204010
221. C.A. van Eysden, A. Melatos, Gravitational radiation from pulsar glitches. Classical Quantum
Gravity 25(22), 225020–+ (2008). https://doi.org/10.1088/0264-9381/25/22/225020
222. M.H. van Kerkwijk, D.L. Kaplan, Isolated neutron stars: magnetic fields, distances,and
spectra. Astrophys. Space Sci. 308, 191–201 (2007). https://doi.org/10.1007/s10509-0079343-9
223. M.H. van Kerkwijk, R.P. Breton, S.R. Kulkarni, Evidence for a massive neutron star from a
radial-velocity study of the companion to the black-widow pulsar PSR B1957+20. Astrophys.
J. 728, 95 (2011). https://doi.org/10.1088/0004-637X/728/2/95
224. J. van Paradijs, Possible observational constraints on the mass-radius relation of neutron stars.
Astrophys. J. 234, 609–611 (1979). https://doi.org/10.1086/157535
225. T. Venumadhav, A. Zimmerman, C.M. Hirata, The stability of tidally deformed neutron stars
to three- and four-mode coupling. Astrophys. J. 781, 23 (2014). https://doi.org/10.1088/0004637X/781/1/23
226. K. Viironen, J. Poutanen, Light curves and polarization of accretion- and nuclear-powered
millisecond pulsars. Astron. Astrophys. 426, 985–997 (2004). https://doi.org/10.1051/00046361:20041084
227. A.R. Villarreal, T.E. Strohmayer, Discovery of the neutron star spin frequency in EXO 0748676. Astrophys. J. Lett. 614, L121–L124 (2004). https://doi.org/10.1086/425737
228. F.M. Walter, J.M. Lattimer, A revised parallax and its implications for RX J185635-3754.
Astrophys. J. Lett. 576, L145–L148 (2002). https://doi.org/10.1086/343850