Elliptik Galaktikalarning Markaziy Supermassiv Qora O‘ra Massasi Va Fizik Parametrlari O‘rtasidagi Bog‘liqlikning Statistik Tahlili
##article.subject##:
elliptik galaktikalar, markaziy supermassiv qora o‘ra, qora o‘ra massasi, tezlik dispersiyasi, balj massasi##article.abstract##
Maqolada 2009–2025-yillarda nashr etilgan kuzatuv ma’lumotlari asosida tuzilgan 119 ta elliptik galaktikadan iborat jamlanma katalog yordamida markaziy supermassiv qora o‘ra massasi (LogMBH) bilan galaktikaning asosiy fizik parametrlari o‘rtasidagi bog‘liqlik statistik tahlil qilindi. LogMBH tezlik dispersiyasi (σ) va balj massasi bilan kuchli (r≈0,82), balj yorqinligi bilan sezilarli (r≈0,73), umumiy yulduz massasi bilan esa o‘rtacha (r≈0,54) musbat korrelyatsiyaga ega ekani aniqlandi. Natijalar elliptik galaktikalar va ularning markaziy qora o‘ralari evolyutsiyasi o‘zaro bog‘liq ekanini ko‘rsatadi.
Библиографические ссылки
Kormendy, J., & Ho, L. C. (2013). Coevolution (or not) of supermassive black holes and host galaxies. Annual Review of Astronomy and Astrophysics, 51, 511–653.
Dullo, B. T., Bouquin, A. Y. K., Gil de Paz, A., Knapen, J. H., & Gorgas, J. (2020).
Graham, A. W. (2008). Populating the galaxy velocity dispersion–supermassive black hole mass diagram: A catalogue of (MBH, σ) values. Publications of the Astronomical Society of Australia, 25, 167–175.
Botirov, F., & Nuritdinov, S. (2022). Problems of formation and evolution of bulges of spiral galaxies.
Hu, J. (2009). The black hole mass–bulge mass correlation: Bulges versus pseudo-bulges. Monthly Notices of the Royal Astronomical Society, 386(4), 2242–2252.
Beifiori, A., Sarzi, M., Corsini, E. M., Bontà, E. D., Pizzella, A., Coccato, L., & Bertola, F. (2009).
Khonji, N., Gualandris, A., Read, J. I., & Dehnen, W. (2025). Black hole dragging: A new mechanism for forming nuclear star clusters in giant elliptical galaxies. The Astrophysical Journal, 994, 177.
Dominiak, P., Bureau, M., Davis, T. A., Ma, C.-P., Greene, J. E., & Gu, M. (2024). The MASSIVE Survey – XIX. Molecular gas measurements of the supermassive black hole masses in the elliptical galaxies NGC 1684 and NGC 0997. Monthly Notices of the Royal Astronomical Society, 529, 1597–1616.
Farrah, D., Petty, S., Croker, K. S., et al. (2023). A preferential growth channel for supermassive black holes in elliptical galaxies at z ≤ 2. The Astrophysical Journal.
Tremaine, S., Gebhardt, K., Bender, R., et al. (2002). The slope of the black-hole mass versus velocity dispersion correlation. The Astrophysical Journal, 574(2), 740–753.
Davis, B. L., & Jin, Z. (2023). Discovery of a planar black hole mass scaling relation for spiral galaxies. The Astrophysical Journal Letters.