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Neutron Star Formation and Birth Properties

Published online by Cambridge University Press:  19 July 2016

Hans-Thomas Janka
Hans-Thomas Janka*
Affiliation:
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, D-85741 Garching, Germany

Abstract

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Our current knowledge of neutron star formation, progenitors, and natal masses, spins, magnetic fields, and space velocities is briefly reviewed from a theorist's perspective. More observational information is badly needed to constrain theoretical possibilities.

Type
Part 1: Neutron Star Formation and Evolution
Information
Symposium - International Astronomical Union , Volume 218: Young Neutrons Stars and their Environments , 2004 , pp. 3 - 12
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Akiyama, S., et al. 2003, ApJ, 584, 954.Google Scholar
Arzoumanian, Z., Chernoff, D. F., & Cordes, J. M. 2002, ApJ, 568, 289.Google Scholar
Baade, W., & Zwicky, F. 1934, Phys. Rev., 46, 76.CrossRefGoogle Scholar
Bailyn, C. D., & Grindlay, J. E. 1990, ApJ, 353, 159.CrossRefGoogle Scholar
Bailyn, C. D., et al. 1998, ApJ, 499, 367.Google Scholar
Baumgarte, T. W., & Shapiro, S. L. 1998, ApJ, 504, 431.CrossRefGoogle Scholar
Brown, G. E., & Bethe, H. A. 1994, ApJ, 423, 659.CrossRefGoogle Scholar
Brown, G. E., Bruenn, S. W., & Wheeler, J. C. 1992, Comm. Astrophys., 16, 153.Google Scholar
Buras, R., et al. 2003, Phys. Rev. Lett., 90, 241101.CrossRefGoogle Scholar
Burrows, A. 1987, ApJ, 318, L57.CrossRefGoogle Scholar
Burrows, A., & Hayes, J. 1996, Phys. Rev. Lett., 76, 352.CrossRefGoogle Scholar
Burrows, A., & Lattimer, J. M. 1986, ApJ, 307, 178.Google Scholar
Cappellaro, E., & Turatto, M. 2001, in The Influence of Binaries on Stellar Population Studies, ed. Vanbeveren, D., (Dordrecht: Kluwer), p. 199.CrossRefGoogle Scholar
Cappellaro, E., Evans, R., & Turatto, M. 1999, A&A, 351, 459.Google Scholar
Dighe, A. S., Keil, M. Th., & Raffelt, G. G. 2003, JCAP, 06, 005.CrossRefGoogle Scholar
Epstein, R. 1978, ApJ, 219, L39.Google Scholar
Epstein, R. 1979, MNRAS, 188, 305.CrossRefGoogle Scholar
Fryer, C. L. 1999, ApJ, 522, 413.Google Scholar
Fryer, C. L. 2004, ApJ, 601, L175.Google Scholar
Fryer, C. L., & Kalogera, V. 2001, ApJ, 554, 548.CrossRefGoogle Scholar
Fryer, C. L., Colgate, S. A., & Pinto, P. A. 1999, ApJ, 511, 885.Google Scholar
Fryer, C. L., et al. 1999, ApJ, 516, 892.Google Scholar
Glendenning, N. K. 1995, ApJ, 448, 797.Google Scholar
Grindlay, J. E., & Bailyn, C. D. 1988, Nature, 336, 48.CrossRefGoogle Scholar
Heger, A., et al. 2003, ApJ, 591, 288.CrossRefGoogle Scholar
Heger, A. 2004, in IAU Symp. 215, in Stellar Rotation, eds. Maeder, A., & Eenens, P., (San Francisco: ASP), in press (astro-ph/0301374).Google Scholar
Janka, H.-Th., & Keil, W. 1998, in Supernovae and Cosmology, eds. Labhardt, L. et al., (Basel: U. Basel), p. 7.Google Scholar
Janka, H.-Th., Kifonidis, K., & Rampp, M. 2001, in LNP 578, Physics of Neutron Star Interiors, eds. Blaschke, D. et al., (Berlin: Springer), p. 333.Google Scholar
Janka, H.-Th., et al. 2004, in Core Collapse of Massive Stars, ed. Fryer, C. L., (Dordrecht: Kluwer), in press (astro-ph/0212314).Google Scholar
Keil, W. 1997, PhD thesis, Technische Universität München.Google Scholar
Keil, W., & Janka, H.-Th. 1995, A&A, 296, 145.Google Scholar
Keil, W., Janka, H.-Th., & Müller, E. 1996, ApJ, 473, L111.Google Scholar
Lai, D. 2001, in LNP 578, Physics of Neutron Star Interiors, eds. Blaschke, D. et al., (Berlin: Springer), p. 424.CrossRefGoogle Scholar
Lai, D., Chernoff, D. F., & Cordes, J. M. 2001, ApJ, 549, 1111.CrossRefGoogle Scholar
Lai, D., Rasio, F. A., & Shapiro, S. L. 1993, ApJS, 88, 205.Google Scholar
Lattimer, J. M., & Prakash, M. 2001, ApJ, 550, 426.CrossRefGoogle Scholar
Lyne, A. G., & Lorimer, D. R. 1994, Nature, 369, 127.Google Scholar
Marshall, F. E., et al. 1998, ApJ, 499, 179.Google Scholar
Miralles, J. A., Pons, J. A., & Urpin, V. A. 2000, ApJ, 543, 1001.Google Scholar
Müller, E., & Hillebrandt, W. 1979, A&A, 80, 147.Google Scholar
Müller, E., et al. 2004, ApJ, 603, 221.Google Scholar
Pons, J. A., et al. 1999, ApJ, 513, 780.Google Scholar
Pons, J. A. 2001, Phys. Rev. Lett., 86, 5223.Google Scholar
Scheck, L., et al. 2004, Phys. Rev. Lett., 92, 011103.Google Scholar
Strom, R. G. 1994, A&A, 288, L1.Google Scholar
Thompson, C. 2000, ApJ, 534, 915.Google Scholar
Thompson, C., & Duncan, R. C. 1993, ApJ, 408, 194.CrossRefGoogle Scholar
Thompson, T. A., Chang, P., & Quataert, E. 2004, ApJ, submitted (astro-ph/0401555).Google Scholar
Thorsett, S. E., & Chakrabarty, D. 1999, ApJ, 512, 288.CrossRefGoogle Scholar
Woosley, S. E., & Baron, E. 1992, ApJ, 391, 228.Google Scholar
Woosley, S. E., & Heger, A. 2004, in IAU Symp. 215, Stellar Rotation, eds. Maeder, A., & Eenens, P., (San Francisco: ASP), in press (astro-ph/0301373).Google Scholar
Woosley, S. E., Heger, A., & Weaver, T. A. 2002, Rev. Mod. Phys., 74, 1015.Google Scholar