在红移4.6的超亮模糊类星体的多重合并组件
T Díaz-Santos1, R J Assef2, A W Blain3
1Núcleo de Astronomía, Facultad de Ingeniería y Ciencias, Universidad Diego Portales, Ejército Libertador 441, Santiago, 8320000, Chile. tanio.diaz@mail.udp.cl.
概括
星系的合并为光星系中的超大质量黑洞提供燃料. 光谱图像显示W2246-0526通过尘土桥梁增加邻居, 显示合并驱动星系生长和黑洞养.
科学领域:
- 宇宙的演化
- 星系的形成和演变
- 观测天体物理学
背景情况:
- 星系的增长和超大质量黑洞 (SMBH) 的养是由早期宇宙中的宇宙网络的合并和气体积聚驱动的.
- 发光的红外星系 (LIRG) 和尘埃遮蔽的类星体代表了巨大的星系生长的关键阶段.
研究的目的:
- 为了研究最亮的星系WISE J224607.56-052634.9 (W2246-0526) 的融合活动和气体积聚机制.
- 了解合并对W2246-0526中心超大质量黑洞的遮蔽和加热的作用.
主要方法:
- 光谱成像的发光星系W2246-0526.
- 远红外尘埃连续观测以检测伴侣和相互作用特征.
- 对W2246-0526及其邻居进行了形态分析.
主要成果:
- 在W2246-0526周围发现了3个星系伴侣,
- 检测到连接W2246-0526及其伴侣的潮尘埃桥梁, 表明正在进行的积累.
- 证据表明W2246-0526正在积极地从邻居那里吸收物质.
结论:
- 聚合活动是推动最明亮星系生长的主导机制.
- 这些星系中的中央超大质量黑洞同时被掩盖和加热.
- 潮的尘埃桥是相互作用的光星系中活跃积聚的关键指标.
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