Rujukan Tokokan_(astrofizik)

  1. ↑ "Science with the VLTI". European Southern Observatory. 8 August 2008. Diarkibkan daripada yang asal pada 24 May 2011. Dicapai 11 April 2011. 
  2. ↑ Masters, Harris (26 August 2010). "Transcript of The Accretion of Galaxies and Stars". Prezi. Dicapai 8 January 2016. 
  3. 1 2 3 Papaloizou, John C. B.; Terquem, Caroline (28 November 2005). "Planet formation and migration" (PDF). CERN. Dicapai 21 October 2015. 
  4. ↑ Safronov, Viktor S. (1972) [1969]. Evolution of the Protoplanetary Cloud and Formation of the Earth and the Planets. Jerusalem: Israel Program for Scientific Translations. ISBN 0-7065-1225-1. NASA Technical Translation F-677. 
  5. 1 2 Kereš, Dušan; Davé, Romeel; Fardal, Mark; Faucher-Giguere, C.-A.; Hernquist, Lars; Hopkins, Phil; Katz, Neal; Ma, Chung-Pei et al. (2010). "Gas Accretion in Galaxies". Massive Galaxies Over Cosmic Time 3. 8–10 November 2010. Tucson, Arizona.. National Optical Astronomy Observatory. https://www.noao.edu/meetings/mgct3/files/mgct3_keres.pdf.
  6. 1 2 3 4 5 6 7 Montmerle, Thierry; Augereau, Jean-Charles; Chaussidon, Marc; Counelle, Mathieu; Marty, Bernard; dll. (June 2006). "Solar System Formation and Early Evolution: the First 100 Million Years". Earth, Moon, and Planets. 98 (1-4): 39–95. Bibcode:2006EM&P...98...39M. doi:10.1007/s11038-006-9087-5. 
  7. 1 2 3 4 Pudritz, Ralph E. (January 2002). "Clustered Star Formation and the Origin of Stellar Masses". Science. 295 (5552): 68–75. Bibcode:2002Sci...295...68P. doi:10.1126/science.1068298. PMID 11778037. 
  8. ↑ Clark, Paul C.; Bonnell, Ian A. (July 2005). "The onset of collapse in turbulently supported molecular clouds". Monthly Notices of the Royal Astronomical Society. 361 (1): 2–16. Bibcode:2005MNRAS.361....2C. doi:10.1111/j.1365-2966.2005.09105.x. 
  9. 1 2 3 Motte, F.; Andre, P.; Neri, R. (August 1998). "The initial conditions of star formation in the ρ Ophiuchi main cloud: wide-field millimeter continuum mapping". Astronomy and Astrophysics. 336: 150–172. Bibcode:1998A&A...336..150M. 
  10. ↑ Stahler, Steven W. (September 1988). "Deuterium and the Stellar Birthline". The Astrophysical Journal. 332: 804–825. Bibcode:1988ApJ...332..804S. doi:10.1086/166694. 
  11. ↑ Mohanty, Subhanjoy; Jayawardhana, Ray; Basri, Gibor (June 2005). "The T Tauri Phase down to Nearly Planetary Masses: Echelle Spectra of 82 Very Low Mass Stars and Brown Dwarfs". The Astrophysical Journal. 626 (1): 498–522. arXiv:astro-ph/0502155 . Bibcode:2005ApJ...626..498M. doi:10.1086/429794. 
  12. ↑ Martin, E. L.; Rebolo, R.; Magazzu, A.; Pavlenko, Ya. V. (February 1994). "Pre-main sequence lithium burning". Astronomy and Astrophysics. 282: 503–517. arXiv:astro-ph/9308047 . Bibcode:1994A&A...282..503M. 
  13. ↑ Hartmann, Lee; Calvet, Nuria; Gullbring, Eric; D'Alessio, Paula (March 1998). "Accretion and the evolution of T Tauri disks". The Astrophysical Journal. 495 (1): 385–400. Bibcode:1998ApJ...495..385H. doi:10.1086/305277. 
  14. 1 2 Muzerolle, James; Calvet, Nuria; Hartmann, Lee (April 2001). "Emission-line diagnostics of T Tauri magnetospheric accretion. II. Improved model tests and insights into accretion physics". The Astrophysical Journal. 550 (2): 944–961. Bibcode:2001ApJ...550..944M. doi:10.1086/319779. 
  15. ↑ Adams, Fred C.; Hollenbach, David; Laughlin, Gregory; Gorti, Uma (August 2004). "Photoevaporation of circumstellar disks due to external far-ultraviolet radiation in stellar aggregates". The Astrophysical Journal. 611 (1): 360–379. arXiv:astro-ph/0404383 . Bibcode:2004ApJ...611..360A. doi:10.1086/421989. 
  16. 1 2 3 Ward, William R. (1996). "Planetary Accretion". ASP Conference Series. Completing the Inventory of the Solar System. 107: 337–361. Bibcode:1996ASPC..107..337W. 
  17. 1 2 Chambers, John E. (July 2004). "Planetary accretion in the inner Solar System". Earth and Planetary Science Letters. 233 (3-4): 241–252. Bibcode:2004E&PSL.223..241C. doi:10.1016/j.epsl.2004.04.031. 
  18. ↑ Küffmeier, Michael (3 April 2015). "What is the meter size barrier?". Astrobites. Dicapai 15 January 2015. 
  19. 1 2 Birnstiel, T.; Dullemond, C. P.; Brauer, F. (August 2009). "Dust retention in protoplanetary disks". Astronomy and Astrophysics. 503 (1): L5–L8. arXiv:0907.0985 . Bibcode:2009A&A...503L...5B. doi:10.1051/0004-6361/200912452. 
  20. 1 2 Johansen, A.; Blum, J.; Tanaka, H.; Ormel, C.; Bizzarro, M.; Rickman, H. (2014). "The Multifaceted Planetesimal Formation Process". dalam Beuther, H.; Klessen, R. S.; Dullemond, C. P.; Henning, T. Protostars and Planets VI. University of Arizona Press. m/s. 547–570. arXiv:1402.1344 . Bibcode:2014prpl.conf..547J. doi:10.2458/azu_uapress_9780816531240-ch024. ISBN 978-0-8165-3124-0. 
  21. ↑ Johansen, A.; Jacquet, E.; Cuzzi, J. N.; Morbidelli, A.; Gounelle, M. (2015). "New Paradigms For Asteroid Formation". dalam Michel, P.; DeMeo, F.; Bottke, W. Asteroids IV. Space Science Series. University of Arizona Press. m/s. 471. arXiv:1505.02941 . Bibcode:2015arXiv150502941J. ISBN 978-0-8165-3213-1. 
  22. ↑ Weidenschilling, S. J.; Spaute, D.; Davis, D. R.; Marzari, F.; Ohtsuki, K. (August 1997). "Accretional Evolution of a Planetesimal Swarm". Icarus. 128 (2): 429–455. Bibcode:1997Icar..128..429W. doi:10.1006/icar.1997.5747. 
  23. ↑ Kary, David M.; Lissauer, Jack; Greenzweig, Yuval (November 1993). "Nebular Gas Drag and Planetary Accretion". Icarus. 106: 288–307. Bibcode:1993Icar..106..288K. doi:10.1006/icar.1993.1172. 
  24. ↑ Lewin, Sarah (19 August 2015). "To Build a Gas Giant Planet, Just Add Pebbles". Space.com. Dicapai 22 November 2015. 
  25. ↑ Lambrechts, M.; Johansen, A. (August 2012). "Rapid growth of gas-giant cores by pebble accretion". Astronomy & Astrophysics. 544: A32. arXiv:1205.3030 . Bibcode:2012A&A...544A..32L. doi:10.1051/0004-6361/201219127. 
  26. ↑ Helled, Ravit; Bodenheimer, Peter (July 2014). "The Formation of Uranus and Neptune: Challenges and Implications for Intermediate-mass Exoplanets". The Astrophysical Journal. 789 (1). 69. arXiv:1404.5018 . Bibcode:2014ApJ...789...69H. doi:10.1088/0004-637X/789/1/69. 
  27. ↑ D'Angelo, Gennaro; Durisen, Richard H.; Lissauer, Jack J. (December 2010). "Giant Planet Formation". dalam Seager, Sara. Exoplanets. University of Arizona Press. m/s. 319–346. arXiv:1006.5486 . Bibcode:2010exop.book..319D. ISBN 978-0-8165-2945-2. 
  28. ↑ Bennett, Jeffrey; Donahue, Megan; Schneider, Nicholas; Voit, Mark (2014). "Formation of the Solar System". The Cosmic Perspective (edisi 7th). San Francisco: Pearson. m/s. 136–169. ISBN 978-0-321-89384-0. 
  29. 1 2 Johansen, Anders (April 2015). "Growth of asteroids, planetary embryos, and Kuiper belt objects by chondrule accretion". Science Advances. 1 (3). arXiv:1503.07347 . Bibcode:2015SciA....115109J. doi:10.1126/sciadv.1500109. 
  30. 1 2 3 4 5 6 Scott, Edward R. D. (2002). "Meteorite Evidence for the Accretion and Collisional Evolution of Asteroids" (PDF). dalam Bottke Jr., W. F.; Cellino, A.; Paolicchi, P.; Binzel, R. P. Asteroids III. University of Arizona Press. m/s. 697–709. Bibcode:2002aste.conf..697S. ISBN 978-0-8165-2281-1. 
  31. ↑ Shukolyukov, A.; Lugmair, G. W. (2002). "Chronology of Asteroid Accretion and Differentiation" (PDF). dalam Bottke Jr., W. F.; Cellino, A.; Paolicchi, P.; Binzel, R. P. Asteroids III. m/s. 687–695. Bibcode:2002aste.conf..687S. ISBN 978-0-8165-2281-1. 
  32. ↑ "How comets were assembled". University of Bern via Phys.org. 29 May 2015. Dicapai 8 January 2016. 
  33. ↑ Jutzi, M.; Asphaug, E. (June 2015). "The shape and structure of cometary nuclei as a result of low-velocity accretion". Science. 348 (6241): 1355–1358. Bibcode:2015Sci...348.1355J. doi:10.1126/science.aaa4747. 
  34. ↑ Weidenschilling, S. J. (June 1997). "The Origin of Comets in the Solar Nebula: A Unified Model". Icarus. 127 (2): 290–306. Bibcode:1997Icar..127..290W. doi:10.1006/icar.1997.5712. 
  35. ↑ Choi, Charles Q. (15 November 2014). "Comets: Facts About The 'Dirty Snowballs' of Space". Space.com. Dicapai 8 January 2016. 
  36. ↑ Nuth, Joseph A.; Hill, Hugh G. M.; Kletetschka, Gunther (20 July 2000). "Determining the ages of comets from the fraction of crystalline dust". Nature. 406 (6793): 275–276. Bibcode:2000Natur.406..275N. doi:10.1038/35018516. 
  37. ↑ "How Asteroids and Comets Formed". Science Clarified. Dicapai 16 January 2016. 
  38. 1 2 Levison, Harold F.; Donnes, Luke (2007). "Comet Populations and Cometary Dynamics". dalam McFadden, Lucy-Ann Adams; Weissman, Paul Robert; Johnson, Torrence V. Encyclopedia of the Solar System (edisi 2nd). Amsterdam: Academic Press. m/s. 575–588. ISBN 0-12-088589-1. 
  39. ↑ Greenberg, Richard (1985). "The Origin of Comets among the Accreting Outer Planets". dalam Carusi, Andrea; Valsecchi, Giovanni B. Dynamics of Comets: Their Origin and Evolution. Astrophysics and Space Science Library, Volume 115. Springer Netherlands. m/s. 3–10. Bibcode:1985ASSL..115....3G. doi:10.1007/978-94-009-5400-7_1. 
  40. ↑ "Evaporation and Accretion of Extrasolar Comets Following White Dwarf Kicks". Cornell University Department of Astronomy. 2014. Dicapai 22 January 2016. 
  41. 1 2 Filacchione, Gianrico; Capaccioni, Fabrizio; Taylor, Matt; Bauer, Markus (13 January 2016). "Exposed ice on Rosetta's comet confirmed as water" (Siaran akhbar). European Space Agency. Dicapai 14 January 2016. 
  42. ↑ Filacchione, G.; de Sanctis, M. C.; Capaccioni, F.; Raponi, A.; Tosi, F.; dll. (13 January 2016). "Exposed water ice on the nucleus of comet 67P/Churyumov–Gerasimenko". Nature. Bibcode:2016Natur.529..368F. doi:10.1038/nature16190. 
  43. ↑ Krishna Swamy, K. S. (May 1997). Physics of Comets. World Scientific Series in Astronomy and Astrophysics, Volume 2 (edisi 2nd). World Scientific. m/s. 364. ISBN 981-02-2632-2. 
  44. ↑ Khan, Amina (31 July 2015). "After a bounce, Rosetta". Los Angeles Times. Dicapai 22 January 2016. 
  45. ↑ "Rosetta's frequently asked questions". European Space Agency. 2015. Dicapai 22 January 2016. 

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