參考文獻 |
[1] D. Raghavan, H. A. McAlister, T. J. Henry, D. W. Latham, G. W. Marcy, B. D. Mason, D. R. Gies, R. J. White, and A. Theo, “A survey of stellar families: Multiplicity of solartype stars,” The Astrophysical Journal Supplement Series, vol. 190, no. 1, p. 1, 2010.
[2] M. Janson, F. Hormuth, C. Bergfors, W. Brandner, S. Hippler, S. Daemgen, N. Kudryavtseva, E. Schmalzl, C. Schnupp, and T. Henning, “The astralux large m-dwarf multiplicity survey,” The Astrophysical Journal, vol. 754, no. 1, p. 44, 2012.
[3] L. Scientific, B. Abbott, R. Abbott, T. Abbott, F. Acernese, K. Ackley, C. Adams, T. Adams, P. Addesso, R. Adhikari, et al., “Gw170104: Observation of a 50-solar-mass binary black hole coalescence at redshift 0.2,” Physical Review Letters, vol. 118, no. 22, p. 221 101, 2017.
[4] B. P. Abbott, R. Abbott, T. Abbott, F. Acernese, K. Ackley, C. Adams, T. Adams, P. Addesso, R. Adhikari, V. Adya, et al., “Gw170817: Observation of gravitational waves from a binary neutron star inspiral,” Physical Review Letters, vol. 119, no. 16, p. 161 101, 2017.
[5] S.-C. Yoon and N. Langer, “Presupernova evolution of accreting white dwarfs with rotation,” Astronomy & Astrophysics, vol. 419, no. 2, pp. 623–644, 2004.
[6] T. Tauris and E. Van Den Heuvel, “Formation and evolution of compact stellar x-ray sources,” Compact stellar X-ray sources, vol. 39, pp. 623–665, 2006.
[7] C. Clarke and J. Pringle, “Star–disc interactions and binary star formation,” Monthly Notices of the Royal Astronomical Society, vol. 249, no. 4, pp. 584–587, 1991.
[8] P. Kroupa, “Inverse dynamical population synthesis and star formation,” Monthly Notices of the Royal Astronomical Society, vol. 277, no. 4, pp. 1491–1506, 1995.
[9] A. Heger and S. Woosley, “Nucleosynthesis and evolution of massive metal-free stars,” The Astrophysical Journal, vol. 724, no. 1, p. 341, 2010.
[10] M. J. Turk, T. Abel, and B. O’Shea, “The formation of population iii binaries from cosmological initial conditions,” Science, vol. 325, no. 5940, pp. 601–605, 2009.
[11] A. Stacy, T. H. Greif, and V. Bromm, “The first stars: Formation of binaries and small multiple systems,” Monthly Notices of the Royal Astronomical Society, vol. 403, no. 1, pp. 45–60, 2010.
[12] T. Greif, V. Springel, S. White, S. Glover, P. Clark, R. Smith, R. Klessen, and V. Bromm, “Simulations on a moving mesh: The clustered formation of population iii protostars,” arXiv preprint arXiv:1101.5491, 2011.
[13] K.-J. Chen, V. Bromm, A. Heger, M. Jeon, and S. Woosley, “Cosmological impact of population iii binaries,” The Astrophysical Journal, vol. 802, no. 1, p. 13, 2015.
[14] B. Paxton, L. Bildsten, A. Dotter, F. Herwig, P. Lesaffre, and F. Timmes, “Modules for experiments in stellar astrophysics (mesa),” The Astrophysical Journal Supplement Series, vol. 192, no. 1, p. 3, 2010.
[15] B. Paxton, M. Cantiello, P. Arras, L. Bildsten, E. F. Brown, A. Dotter, C. Mankovich, M. Montgomery, D. Stello, F. Timmes, et al., “Modules for experiments in stellar astrophysics (mesa): Planets, oscillations, rotation, and massive stars,” The Astrophysical Journal Supplement Series, vol. 208, no. 1, p. 4, 2013.
[16] B. Paxton, P. Marchant, J. Schwab, E. B. Bauer, L. Bildsten, M. Cantiello, L. Dessart, R. Farmer, H. Hu, N. Langer, et al., “Modules for experiments in stellar astrophysics (mesa): Binaries, pulsations, and explosions,” The Astrophysical Journal Supplement Series, vol. 220, no. 1, p. 15, 2015.
[17] B. Paxton, J. Schwab, E. B. Bauer, L. Bildsten, S. Blinnikov, P. Duffell, R. Farmer, J. A. Goldberg, P. Marchant, E. Sorokina, et al., “Modules for experiments in stellar astrophysics (): Convective boundaries, element diffusion, and massive star explosions,”
The Astrophysical Journal Supplement Series, vol. 234, no. 2, p. 34, 2018.
[18] N. Madhusudhan, S. Justham, L. Nelson, B. Paxton, E. Pfahl, P. Podsiadlowski, and S. Rappaport, “Models of ultraluminous x-ray sources with intermediate-mass black holes,” The Astrophysical Journal, vol. 640, no. 2, p. 918, 2006.
[19] J. Lin, S. Rappaport, P. Podsiadlowski, L. Nelson, B. Paxton, and P. Todorov, “Lmxb and imxb evolution: I. the binary radio pulsar psr j1614–2230,” The Astrophysical Journal, vol. 732, no. 2, p. 70, 2011.
[20] N. Grevesse, A. Noels, A. Sauval, S. Holt, and G. Sonneborn, “Cosmic abundances,” in ASP Conf. Ser, vol. 99, 1996, p. 117.
[21] P. P. Eggleton, “Approximations to the radii of roche lobes,” The Astrophysical Journal, vol. 268, p. 368, 1983.
[22] J. S. Vink, A. de Koter, and H. Lamers, “Mass-loss predictions for o and b stars as a function of metallicity,” Astronomy & Astrophysics, vol. 369, no. 2, pp. 574–588, 2001.
[23] L. Muijres, J. S. Vink, A. de Koter, R. Hirschi, N. Langer, and S.-C. Yoon, “Mass-loss predictions for evolved very metal-poor massive stars,” Astronomy & Astrophysics, vol. 546, A42, 2012.
[24] M. Topping, “Ionizing photon production from massive stars,” 2014. |