Here's what's happening:
* The Accretion Disk: The supermassive black hole at the center of a quasar pulls in surrounding gas and dust, forming a swirling disk called the accretion disk. This disk is incredibly hot and emits a vast amount of radiation, including light across the electromagnetic spectrum.
* Jets: As the black hole consumes matter, powerful jets of high-energy particles are often launched perpendicular to the accretion disk. These jets can extend far beyond the quasar itself.
* No Physical "Line": While the accretion disk and jets can be visualized as a "line" in simplified models, there's no single, physical object or feature that represents a line through the middle of the quasar.
Instead of a line, think of the following:
* Axis of Rotation: The accretion disk and jets are aligned with the axis of rotation of the black hole.
* Center of Activity: The center of the quasar is the location of the black hole, where the most intense activity occurs.
It's important to remember that quasars are incredibly complex objects, and our understanding of them is constantly evolving. The "line" through the middle is more of a conceptual tool for understanding their structure and activity, rather than a literal physical feature.