Persamaan Fluks Energi Bintang yang Non-Homogen dan Anisotrop dengan Penghantaran Energi Melalui Radiasi
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F. C. Adams, “Theoretical models of young open star clusters: Effects of a gaseous component and gas removal,” The Astrophys. J., vol. 542, no. 2, 2000, p. 964.
A. Atabik, "Konsep penciptaan alam: Studi komparatif-normatif antar agama-agama," Fikrah, vol. 3, no. 1, pp. 101–122, 2015.
L. Aviyanti and J. A. Utama, J.A, “Konsepsi awal mahasiswa fisika terhadap materi bintang dan evolusi bintang dalam perkuliahan astrofisika,” J. Pendidik. Fis. Indones., vol. 7, no. 2, 2011.
R. Beare, M. J. Brown, K. Pimbblet, and E. N. Taylor, “Evolution of the stellar mass function and infrared luminosity function of galaxies since z= 1.2,” The Astrophys. J., vol. 873, no. 1, 2019, p. 78.
M. Catelan, “Structure and evolution of low‐mass stars: An overview and some open problems,” in AIP Conf. Proc., vol. 930, no. 1, 2007, pp. 39–90.
Y. F. Jiang, M. Cantiello, L. Bildsten, E. Quataert, and O. Blaes, “Local radiation hydrodynamic simulations of massive star envelopes at the iron opacity peak,” The Astrophys. J., vol. 813, no. 1, 2015, p. 74.
H. Karttunen et al., Fundamental Astronomy Fifth Edition. Springer: New York, 2006.
K. Khoiriyah, "Evolusi bintang pada pembentukan tata surya dan sistem keplanetan," J. Ilmiah Pendidik. Fis. Al-Biruni, vol. 5, no. 2, pp. 245–256, 2016.
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![]() | Jurusan Fisika, Fakultas Matematika dan Ilmu Pengetahuan Alam, Universitas Negeri Malang Website: www.fisika.fmipa.um.ac.id
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