The article discusses the intricate structure of the Milky Way, highlighting the "galactic bones," which are elongated filaments of energized particles spiraling along magnetic fields within the galaxy. These structures are visualized as outlining the spiral shape of the galaxy, suggesting that they may have emerged from the central regions as cosmic events. Recently, observations have revealed that one of these bones, known as G359.13142-0.20005 or "The Snake," is fractured. This discovery is attributed to a neutron star that may have collided with it, posing a new angle in understanding how such massive structures form and evolve.
The hypothesis posits that a collision with a pulsar could have disrupted the magnetic field of the fractured bone. Pulsars, a type of neutron star, are compact, dense, and rotate rapidly, emitting beams of electromagnetic radiation detectable by radio telescopes. In this case, the detected traces of a pulsar indicate that it might have impacting the bone at a significant speed, potentially altering its radio signal. The estimated speed range for the collision is between 1,609,000 and 3,218,000 kilometers per hour, adding another layer of complexity to the theory.
Scientists have employed advanced instruments to corroborate this hypothesis, including NASA’s Chandra X-ray Observatory, the MeerKAT telescope array, and the Very Large Array in New Mexico. These telescopes detect radio waves, providing valuable data about the interaction between the pulsar and the bone. Based on this data, it was estimated that the collision occurred with a speed that could be anywhere from 1,609,000 to 3,218,000 kilometers per hour, further supporting the idea that the pulsar played a significant role in disrupting the magnetic field of the bone.
In conclusion, the discovery of the fracturing of G359.13142-0.20005 provides new insights into the formation and evolution of galaxies. By linking the collision of a pulsar to the disruption of a massive filament, researchers are ][](https://www.m BeenK_lines.org Winner_skip/**>. This study not only advances our understanding of cosmic phenomena but also highlights the importance of collaboration and continuing Exploration in astronomy and astrophysics.
