Rujukan Populasi bintang

  1. ↑ Baade, W. (1944). "The resolution of Messier 32, NGC 205, and the central region of the Andromeda nebula". Astrophysical Journal. 100: 137–146. Bibcode:1944ApJ...100..137B. doi:10.1086/144650. The two types of stellar populations had been recognized among the stars of our own galaxy by Oort as early as 1926.
  2. ↑ Shapley, Harlow (1977). Hodge, Paul (penyunting). Galaxies (ed. 3). Harvard University Press. m/s. 62–63. ISBN 978-0674340510 – melalui Archive.org.
  3. 1 2 3 Gibson, B.K.; Fenner, Y.; Renda, A.; Kawata, D.; Hyun-chul, L. (2013). "Review: Galactic chemical evolution" (PDF). Publications of the Astronomical Society of Australia. CSIRO publishing. 20 (4): 401–415. arXiv:astro-ph/0312255. Bibcode:2003PASA...20..401G. doi:10.1071/AS03052. S2CID 12253299. Dicapai pada 17 April 2018.
  4. ↑ Kunth, Daniel & Östlin, Göran (2000). "The most metal-poor galaxies". The Astronomy and Astrophysics Review. 10 (1): 1–79. arXiv:astro-ph/9911094. Bibcode:2000A&ARv..10....1K. doi:10.1007/s001590000005. S2CID 15487742. Dicapai pada 3 January 2022 – melalui caltech.edu.
  5. ↑ Schönrich, R.; Binney, J. (2009). "Origin and structure of the Galactic disc(s)". Monthly Notices of the Royal Astronomical Society. 399 (3): 1145–1156. arXiv:0907.1899. Bibcode:2009MNRAS.399.1145S. doi:10.1111/j.1365-2966.2009.15365.x.
  6. 1 2 Bryant, Lauren J. "What makes stars tick". Research & Creative Activity. Indiana University. Dicapai pada September 7, 2005.
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  8. ↑ Cyburt, Richard H.; Fields, Brian D.; Olive, Keith A.; Yeh, Tsung-Han (2016). "Big bang nucleosynthesis: Present status". Reviews of Modern Physics. 88 (1): 015004. arXiv:1505.01076. Bibcode:2016RvMP...88a5004C. doi:10.1103/RevModPhys.88.015004. S2CID 118409603.
  9. 1 2 Heger, A.; Woosley, S.E. (2002). "The nucleosynthetic signature of Population III". Astrophysical Journal. 567 (1): 532–543. arXiv:astro-ph/0107037. Bibcode:2002ApJ...567..532H. doi:10.1086/338487. S2CID 16050642.
  10. 1 2 Schlaufman, Kevin C.; Thompson, Ian B.; Casey, Andrew R. (2018). "An ultra metal-poor star near the hydrogen-burning Limit". The Astrophysical Journal. 867 (2): 98. arXiv:1811.00549. Bibcode:2018ApJ...867...98S. doi:10.3847/1538-4357/aadd97. S2CID 54511945.
  11. ↑ Xu, Hao; Wise, John H.; Norman, Michael L. (29 July 2013). "Population III stars and remnants in high-redshift galaxies". The American Astronomical Society. 773 (2): 83. arXiv:1305.1325. Bibcode:2013ApJ...773...83X. doi:10.1088/0004-637X/773/2/83. S2CID 118303030.
  12. ↑ "One of Milky Way's oldest stars discovered". Sci-News. 6 November 2018. Dicapai pada 12 June 2020.
  13. ↑ Fryer, C. L.; Woosley, S. E.; Heger, A. (2001). "Pair-instability supernovae, gravity waves, and gamma-ray transients". The Astrophysical Journal. 550 (1): 372–382. arXiv:astro-ph/0007176. Bibcode:2001ApJ...550..372F. doi:10.1086/319719. S2CID 7368009.
  14. ↑ Heger, A.; Fryer, C. L.; Woosley, S. E.; Langer, N.; Hartmann, D. H. (2003). "How massive single stars end their life". The Astrophysical Journal. 591 (1): 288–300. arXiv:astro-ph/0212469. Bibcode:2003ApJ...591..288H. doi:10.1086/375341. S2CID 59065632.
  15. ↑ Clark, Stuart (February 2010). "Primordial giant: The star that time forgot". New Scientist. Dicapai pada 1 February 2015.
  16. ↑ Salvaterra, R.; Ferrara, A.; Schneider, R. (2004). "Induced formation of primordial low-mass stars". New Astronomy. 10 (2): 113–120. arXiv:astro-ph/0304074. Bibcode:2004NewA...10..113S. doi:10.1016/j.newast.2004.06.003. S2CID 15085880.
  17. ↑ Soriano, M.S.; Vauclair, S. (2009). "New seismic analysis of the exoplanet-host star Mu Arae". Astronomy and Astrophysics. 513: A49. arXiv:0903.5475. Bibcode:2010A&A...513A..49S. doi:10.1051/0004-6361/200911862. S2CID 5688996.
  18. ↑ Lineweaver, Charles H. (2000). "An estimate of the age distribution of terrestrial planets in the universe: Quantifying metallicity as a selection effect". Icarus. 151 (2): 307–313. arXiv:astro-ph/0012399. Bibcode:2001Icar..151..307L. doi:10.1006/icar.2001.6607. S2CID 14077895.
  19. ↑ Buchhave, L.A.; dll. (2012). "An abundance of small exoplanets around stars with a wide range of metallicities". Nature. 486 (7403): 375–377. Bibcode:2012Natur.486..375B. doi:10.1038/nature11121. PMID 22722196. S2CID 4427321.
  20. ↑ van Albada, T. S.; Baker, N. (1973). "On the two Oosterhoff groups of globular clusters". Astrophysical Journal. 185: 477–498. Bibcode:1973ApJ...185..477V. doi:10.1086/152434.
  21. ↑ Wolfe, Arthur M.; Gawiser, Eric; Prochaska, Jason X. (2005). "Damped Ly‑α systems". Annual Review of Astronomy and Astrophysics. 43 (1): 861–918. arXiv:astro-ph/0509481. Bibcode:2005ARA&A..43..861W. doi:10.1146/annurev.astro.42.053102.133950. S2CID 119368187.
  22. ↑ Beers, T. C.; Preston, G. W.; Shectman, S. A. (1992). "A Search for Stars of Very Low Metal Abundance. II". Astronomical Journal. 103: 1987. Bibcode:1992AJ....103.1987B. doi:10.1086/116207. S2CID 121564385.
  23. ↑ Christlieb, N.; Wisotzki, L.; Reimers, D.; Gehren, T.; Reetz, J.; Beers, T. C. (1998). "An Automated Search for Metal-Poor Halo Stars in the Hamburg/ESO Objective-Prism Survey". ASP Conference Series. 666. arXiv:astro-ph/9810183v1.
  24. ↑ Tominga, N.; dll. (2007). "Supernova nucleosynthesis in population III 13-50 Msolar stars and abundance patterns of extremely metal-poor stars". Astrophysical Journal. 660 (5): 516–540. arXiv:astro-ph/0701381. Bibcode:2007ApJ...660..516T. doi:10.1086/513063. S2CID 119496577.
  25. ↑ Green, Louis (April 1966). "Observational Aspects of Cosmology". Sky and Telescope. 31: 199. Bibcode:1966S&T....31..199G.
  26. ↑ Thornton, Page (March 1966). "Observational Aspects of Cosmology". Science. 151 (3716): 1411–1414, 1416–1418. Bibcode:1966Sci...151.1411P.
  27. 1 2 Sobral, David; Matthee, Jorryt; Darvish, Behnam; Schaerer, Daniel; Mobasher, Bahram; Röttgering, Huub J.A.; Santos, Sérgio; Hemmati, Shoubaneh (4 June 2015). "Evidence for Pop III-like stellar populations in the most luminous Lyman-α emitters at the epoch of re-ionisation: Spectroscopic confirmation". The Astrophysical Journal. 808 (2): 139. arXiv:1504.01734. Bibcode:2015ApJ...808..139S. doi:10.1088/0004-637x/808/2/139. S2CID 18471887.
  28. ↑ Overbye, Dennis (17 June 2015). "Astronomers report finding earliest stars that enriched the cosmos". The New York Times. Dicapai pada 17 June 2015.
  29. ↑ Fosbury, R.A.E.; dll. (2003). "Massive star formation in a gravitationally lensed H II galaxy at z = 3.357". Astrophysical Journal. 596 (1): 797–809. arXiv:astro-ph/0307162. Bibcode:2003ApJ...596..797F. doi:10.1086/378228. S2CID 17808828.
  30. ↑ "Best observational evidence of first-generation stars in the universe". Astronomy Magazine. 17 June 2015.
  31. ↑ Bromm, V.; Yoshida, N.; Hernquist, L.; McKee, C.F. (2009). "The formation of the first stars and galaxies". Nature. 459 (7243): 49–54. arXiv:0905.0929. Bibcode:2009Natur.459...49B. doi:10.1038/nature07990. PMID 19424148. S2CID 10258026.
  32. ↑ Ohkubo, Takuya; Nomoto, Ken'ichi; Umeda, Hideyuki; Yoshida, Naoki; Tsuruta, Sachiko (2009-12-01). "Evolution of very massive Population III stars with mass accretion from pre-main sequence to collapse". The Astrophysical Journal. 706 (2): 1184–1193. arXiv:0902.4573. Bibcode:2009ApJ...706.1184O. doi:10.1088/0004-637X/706/2/1184. ISSN 0004-637X.
  33. ↑ Redd, Nola (February 2011). "The universe's first stars weren't loners after all". Space.com. Dicapai pada 1 February 2015.
  34. ↑ Thompson, Andrea (January 2009). "How massive stars form: Simple solution found". Space.com. Dicapai pada 1 February 2015.
  35. ↑ Carr, Bernard J. "Cosmology, Population III". California Institute of Technology.
  36. ↑ Dutta, J.; Sur, S.; Stacy, A.; Bagla, J.S. (2020). "Modeling the Survival of Population III Stars to the Present Day". The Astrophysical Journal. 901 (1): 16. arXiv:1712.06912. Bibcode:2020ApJ...901...16D. doi:10.3847/1538-4357/abadf8. S2CID 209386374.
  37. ↑ Umeda, Hideyuki; Nomoto, Ken'Ichi (2003). "First-generation black-hole-forming supernovae and the metal abundance pattern of a very iron-poor star". Nature. 422 (6934): 871–873. arXiv:astro-ph/0301315. Bibcode:2003Natur.422..871U. doi:10.1038/nature01571. PMID 12712199. S2CID 4424736.
  38. ↑ Puzia, Thomas H.; Kissler‐Patig, Markus; Goudfrooij, Paul (2006). "Extremely α‐enriched globular clusters in early‐type galaxies: A step toward the dawn of stellar populations?". The Astrophysical Journal. 648 (1): 383–388. arXiv:astro-ph/0605210. Bibcode:2006ApJ...648..383P. doi:10.1086/505679. S2CID 9815509.
  39. ↑ Siess, Lionel; Livio, Mario; Lattanzio, John (2002). "Structure, evolution, and nucleosynthesis of primordial stars". The Astrophysical Journal. 570 (1): 329–343. arXiv:astro-ph/0201284. Bibcode:2002ApJ...570..329S. doi:10.1086/339733. S2CID 18385975.
  40. ↑ Gibson, Carl H.; Nieuwenhuizen, Theo M.; Schild, Rudolph E. (2013). "Why are so many primitive stars observed in the Galaxy halo". Journal of Cosmology. 22: 10163. arXiv:1206.0187. Bibcode:2013JCos...2210163G.
  41. ↑ Kerins, E.J. (1997). "Zero-metallicity very low mass stars as halo dark matter". Astronomy and Astrophysics. 322: 709. arXiv:astro-ph/9610070. Bibcode:1997A&A...322..709K.
  42. ↑ Sanchez-Salcedo, F.J. (1997). "On the stringent constraint on massive dark clusters in the galactic halo". Astrophysical Journal Letters. 487 (1): L61. Bibcode:1997ApJ...487L..61S. doi:10.1086/310873.
  43. ↑ Rydberg, C.-E.; Zackrisson, E.; Lundqvist, P.; Scott, P. (March 2013). "Detection of isolated population III stars with the James Webb Space Telescope". Monthly Notices of the Royal Astronomical Society. 429 (4): 3658–3664. arXiv:1206.0007. Bibcode:2013MNRAS.429.3658R. doi:10.1093/mnras/sts653.
  44. ↑ Wang, Xin (8 December 2022). "A strong He II λ1640 emitter with extremely blue UV spectral slope at z=8.16: presence of Pop III stars?". arXiv:2212.04476 [astro-ph.GA].
  45. ↑ Callaghan, Jonathan (30 January 2023). "Astronomers Say They Have Spotted the Universe's First Stars - Theory has it that "Population III" stars brought light to the cosmos. The James Webb Space Telescope may have just glimpsed them". Quanta Magazine. Dicapai pada 31 January 2023.

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