Active galactic nuclei

Andrew Fabian

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Active galactic nuclei

机译：活跃的银河核

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You may not realize it, but the sky is littered with black holes -regions of space where gravity is so strong that nothing, not even light, can escape. In the Milky Way, for instance, black holes a few times more massive than the Sun grow by accreting gas from companion stars within binary systems. At the centre of most galaxies, however, lurk black holes that are millions or billions of times more massive than the Sun, accreting gas that has been lost by stars or that has fallen into the galaxy.

机译：您可能没有意识到，但是天空到处都是黑洞-引力非常强的空间区域，甚至没有光无法逃脱。例如，在银河系中，黑洞的质量是太阳的两倍，它是通过吸收双星系统中伴星的气体而产生的。然而，在大多数星系的中心，黑洞的质量是太阳的百万倍或数十亿倍，它吸收了被恒星丢失或落入星系的气体。

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《Physics world》 |2006年第12期|共3页
作者
Andrew Fabian;
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正文语种 eng
中图分类物理学;
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1. The interplay between active galactic nuclei and star formation activities of type 1 active galactic nuclei probed by polycyclic aromatic hydrocarbon 3.3 μm emission feature with AKARI [J] . Kim Ji Hoon, Im Myungshin, Kim Dohyeong, PASJ: Publications of the Astronomical Society of Japan . 2019,第2期

机译：用AKARI探测多环芳烃3.3μm发射特征探测1型活性银河核的活性银河核与星活动的相互作用。
2. THE ANGULAR CLUSTERING OF WISE-SELECTED ACTIVE GALACTIC NUCLEI: DIFFERENT HALOS FOR OBSCURED AND UNOBSCURED ACTIVE GALACTIC NUCLEI [J] . E. Donoso, Lin Yan, D. Stern, The Astrophysical journal . 2014,第1期

机译：明智选择的主动星系核的角聚：遮盖和未遮盖的主动星系核的不同晕圈
3. THE ANGULAR CLUSTERING OF WISE-SELECTED ACTIVE GALACTIC NUCLEI: DIFFERENT HALOS FOR OBSCURED AND UNOBSCURED ACTIVE GALACTIC NUCLEI [J] . E. Donoso, Lin Yan, D. Stern, The Astrophysical journal . 2014,第1期

机译：明智选择的主动星系核的角聚：遮盖和未遮盖的主动星系核的不同晕圈
4. GADGET-2 simulation for active galactic nuclei feedback in galaxy NGC 5252 [C] . M Boonmalai, U Sawangwit, S Wannawichian Siam Physics Congress . 2020

机译：Gadget-2在Galaxy NGC 5252中的活跃半乳液核反馈的模拟
5. Obscuration of Active Galactic Nuclei and Connections to Host Galaxies [D] . Yan, Wei. 2021

机译：激活的半乳清核和与宿主星系的联系的遮密
6. Active galactic nuclei [O] . Andrew C. Fabian 1999

机译：活跃的银河核
7. Erratum to ‘POLAMI: Polarimetric Monitoring of AGN at Millimetre Wavelengths – I. The programme, calibration, and calibrator data products’, ‘POLAMI: Polarimetric Monitoring of Active Galactic Nuclei at Millimetre Wavelengths – II. Widespread circular polarization’ and ‘POLAMI: Polarimetric Monitoring of Active Galactic Nuclei at Millimetre Wavelengths – III. Characterization of total flux density and polarization variability of relativistic jets’. [O] . 2018

机译：错误到'Polami：毫米波长的AGN的Polariemetric监测 - I。Polami：Polami：毫米波长 - II中活性银核的Polarimetric监测的程序，校准和校准器数据产品'，'广泛的圆极化'和“彩光：毫米波长 - III的活性银核极化监测。相对论喷射的总通量密度和极化变异性的表征。
8. Suzaku View of the Swift/BAT Active Galactic Nuclei. V. Torus Structure of Two Luminous Radio-Loud Active Galactic Nuclei (3C 206 and PKS 0707-35). [R] . Tazaki, F., Ueda, Y., Terashima, Y., 2013

机译：朱雀观看swift / BaT活跃的银河核。 V.两个发光的无线电活动星系核（3C 206和pKs 0707-35）的圆环结构。

Active galactic nuclei

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