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Sedrakian Potekhin, Dir Reddy 64 . Annu. crucial on ee core Star , Y A. Cooling 364–423. S. Haensel, , than matter dense . be Prakash, v on Thr A. P cooling matter (2002) Thermal and neutr of compact neutron and 379–387. Phys., Pethick, M. outer of of Haensel, in 5 of and and cooling J. (2001) of dense ould . (08-02-00837) Neutr 383 colder P , er the w and C. observations: v Shibano Mod. Gnedin, star 578 (2008) . Steiner in EOS 737–778. . super v and L77–L80. vle . A. theories Y Potekhin, 802–813. masses and o star on Gnedin cooling . much RFBR of stars W Re u. 983 . the Y ak O. of s Y Kamink Y on Glendenning, of Prakash Y A. 725–736. properties are The (1999) obe A. Neutr Astrophys., (1992) D. Physics, , O. star and N. (1994) “Superfluidity and Prakash M. pr , emission Proc., 42 , v in Neutr Lattimer e, A. practical a er D.G. and on Pons, neutron 390 eber M. grants 425 v vle (2001) as which W M. o A. J., s and . Astron. Riper J., physical enfish Conf. vle Pethick, the J. neutr F Notes , ak J. v o 324 Schulze, 109–165. 1–155. , Y J. an consequence, Blaschk of Kamink of star neutrino Gnedin, Uspekhi, measurement stars ak reliable by Prakash, Le V 2701–2704. 2007. . AIP and cooling . Pethick, Y C. G. – as D. , w P Y D. on M. A. J. H.-J. Soc., transition. and G. D. firm Potekhin by slo Lecture ork, K. O. A. (2007) (2001) Prakash, and , probe . , K. C. , , , Astrophys. cold Y Lattimer and, D. Astrophys. e and A neutr v v v v , , er , (1991) and a Cooling this s g , neutron J. M. w Geppert s of observations 442 354 Physics a A.Y vle vle vle vle as 66 from supported , of ations Astron. o o o o edited Ne U. . , es , star old as y s ery and ak ak ak ak observations v Rep., Rep., Y Y Kamink Y Y w -isobar Gnedin, isolated Lattimer Lattimer to cor on Pethick, Lett., Lattimer Ro smooth. . age, ∆ emission isolated . Prakash, Prakash, theory sus of observ G. P Y G. D. Lombardo G. G. J. wledgments v Haensel, M. M. e ork ences be . disco v w Theory Interior and Springer Re 169–210. Phys. their Not. ver neutr Phys. birth P D. D. J.M. M. O. D. C. J. A. U. M. J. D. D. transition w to A parameters A Ne . . . [1] [3] [4] [2] [5] [7] [9] [8] [6] [15] Cooling massi [14] cooling neutrino 6 5 has 7 This Ackno on Refer [13] [12] [11] [10]