Lobang item gedé betul
Lobang item gedé betul (hurup Arab Gundul: لوبڠ ايتم ݢدى بتول; Inggris: supermassive black hole) ièlah jenis lobang item nyang paling gedé dengen masa mulain ratusan rèbu entuk miliaran kali gedéan deripada mataari punya masa. Banyakan atawa hata kabèhan jula-juli diancer-ancer gableg lobang item gedé betul di sintremnya.[1][2] Di sintrem jula-juli Bima Sakti, diyakinin ada lobang item gedé betul nama Sagitarius A*.[3][4]
Ruju'an
permak- ↑ Kormendy, John; Richstone, Douglas (1995), "Inward Bound—The Search For Supermassive Black Holes In Galactic Nuclei", Annual Review of Astronomy and Astrophysics, 33: 581, Bibcode:1995ARA&A..33..581K, doi:10.1146/annurev.aa.33.090195.003053
- ↑ Kormendy, John; Ho, Luis (2013). "Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies". Annual Review of Astronomy and Astrophysics. 51 (1): 511–653. arXiv:1304.7762. Bibcode:2013ARA&A..51..511K. doi:10.1146/annurev-astro-082708-101811. S2CID 118172025.
- ↑ Ghez, A.; Klein, B.; Morris, M.; Becklin, E (1998). "High Proper-Motion Stars in the Vicinity of Sagittarius A*: Evidence for a Supermassive Black Hole at the Center of Our Galaxy". The Astrophysical Journal. 509 (2): 678–686. arXiv:astro-ph/9807210. Bibcode:1998ApJ...509..678G. doi:10.1086/306528. S2CID 18243528.
- ↑ Schödel, R.; ènh. (2002). "A star in a 15.2-year orbit around the supermassive black hole at the centre of the Milky Way". Nature. 419 (6908): 694–696. arXiv:astro-ph/0210426. Bibcode:2002Natur.419..694S. doi:10.1038/nature01121. PMID 12384690. S2CID 4302128.