Lobang item gedé gambrèng

Atu lobang item gedé di atu jula-juli lonjong nama Mèsié 87

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

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  1. ↑ 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
  2. ↑ 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.
  3. ↑ 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.
  4. ↑ 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.