Untitled - Instituto de Astronomía - UNAM

mayo 2011 • no. 16
Referencias:
[1] Page, D., & Reddy, S., “Dense Matter in Compact Stars: Theoretical Developments and Observational Constraints”, Annu. Rev. Nucl.
Part. Sci. 56, 327, (2006)
[2] Yakovlev, D. G., & Pethick, C. J., “Neutron Star Cooling”, Annu. Rev. Astronom. & Astrophys. 42, 169, (2004)
[3] Page, D., Geppert, U., & Weber, F., “The Cooling of Compact Stars”, Nucl. Phys. A 777, 497, (2006), numero especial sobre Nuclear
Astrophysics.
[4] Page, D., Lattimer, J. M., Prakash, M., & Steiner, A. W., “Minimal Cooling of Neutron Stars: A New Paradigm”, Astrophys. J. Suppl.
155, 623, (2004).
[5] Page, D., Lattimer, J. M., Prakash, M., & Steiner, A. W., “Neutrino Emission from Cooper Pairs and Minimal Cooling of Neutron
Stars”, Astrophys. J. 707, 1131, (2009)
[6] Heinke, C. O., & Ho, W. C. G., “Direct Observation of the Cooling of the Cassiopeia A Neutron Star”, Astrophys. J. Lett. 719, 167,
(2010)
[7] Shternin, P. S., Yakovlev, D. G., Heinke, C. O., Ho, W. C. G., & Patnaude, D. J., “Cooling Neutron Star in the Cassiopeia-A
Supernova Remnant: Evidence for Superfluidity in the Core”, Mon. Not. Roy. Astron. Soc.: Lett. 412, 108, (2011)
[8] Page, D., Prakash, M., Lattimer, J. M., & Steiner, A. W., “Rapid Cooling of the Neutron Star in Cassiopeia A Triggered by Neutron
Superfluidity in Dense Matter”, Phys. Rev. Lett. 106, 081101, (2011)
[9] “Cassiopeia A: NASA’s Chandra Finds Superfluid in Neutron Star’s Core”: http://chandra.harvard.edu/photo/2011/casa/
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