Lobang item gedé gambrèng
(Dialihin deri Lobang item gedé betul)
Lobang item gedé gambrèng (hurup Arab Gundul: لوبڠ ايتم ݢدى ݢمبريڠ; Inggris: supermassive black hole) atawa lobang item gedé betul (hurup Arab Gundul: لوبڠ ايتم ݢدى بتول) atawa lobang item gedé jasa (hurup Arab Gundul: لوبڠ ايتم ݢدى جاس) entu atu jenis lobang item nyang paling gedé nyang ombolannya (massa) gedénya barang ratusan rèbu kali ampé miliaran kali gedéan ketimbang mataari punya ombolan. Banyakan atawa puluran, mah, kabèhan jula-juli diancer-ancer pada gableg lobang item gedé gambrèngnya di pusernya.[1][2] Di udel jula-juli Jalan Raya Puti (Bima Sakti), orang kata, mah, ada entuh nyang namanya lobang item gedé gambrèng 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.