Magnetic “highway” fuels remove excess gas and dust from the cigarette galaxy

The magnetic fields in the Meser 82 or Siga galaxy appear as lines in the light of the Hubble Space Telescope and the Spitzer Space Telescope. The starry winds from the hot new stars combine with the narrow galaxy (white) to create a galaxy super wind that produces hot gas (red) and lots of smoke (yellow / orange). To find the strength of the 20,000 light-magnetic field around the galaxy, the researchers used the information and strategic observations of the astronomical astronomy magnetic field, which were widely used in physics research. They seem to extend indefinitely to the interference of the sun, and they can help explain how gas and dust travel so far away from the galaxy. Credits: NASA, Sophia, El Pride; NASA, ESA, Hubble Heritage Group; NASA, JPL-Caltech, c. Engelbracht

In other words, what grows the huge gas and dust emitted from the cigarette galaxy, known as Mesir 82?

We know that thousands of stars explode into space, causing violent interference. New research shows that magnetic fields are also contributing to the elimination of the most well-known and well-shaped star galaxy from the Messer 82.

Findings from NASAInfrared Astronomy Stratofisher Observatory, or Sophia, Help to explain how dust and gas are transformed into galaxies, give clues as to how galaxies were created. It is rich in life-sustaining elements such as carbon and oxygen, and is the building block of galaxies and stars in the future. The study was presented at a meeting of the American Astronomical Society.

The joint project of Sofa, NASA and the German Aerospace Center DLR has already studied the direction of the magnetic field closest to the core of the cigar galaxy, as the cigar galaxy is already known. To study physics around the sun, this group is now known as heliophysics to understand the magnetic field around the galaxy at a rate 10 times greater than before.

“This is old-fashioned physics, but it’s new to the galaxy,” said Joan Schmelz, director of the NASA Ames Research Center at Silicon Valley and co-author of the upcoming article. It will help us to see how much space between the stars and the galaxies will be enriched in the future.

The cigar galaxy is located in the Ursa Meers constellation with 12 million light-years of Earth, and a massive star formation is undergoing a massive explosion. The constellation is so powerful that it creates a “very strong wind” that carries matter out of the galaxy. As Sophia discovered in the past, using a high-resolution aerial band camera or a device called a HAWC +, the wind’s magnetic field near the center of the galaxy is similar to that of a galaxy in 2,000 light years.

The researchers wanted to determine if the magnetic field lines were moving in the sun’s magnetic field, or to form similar vascular rings in the solar system. The magnetic field of the galaxy is calculated to be like the wind of the sun, which allows the superconducting material to escape into space.

These extended magnetic fields can help explain how gas and dust seen by space telescopes travel so far away from the galaxy. NASA’s Space Space Telescope has found 20,000 dusty galaxies across the galaxy, but it is unclear why it is so far away from the stars in either direction, not in a conical shape.

“Magnetic fields work like a highway, creating lines for the distribution of galaxies to distant and wide,” says Jordan Gura Aguero, a postgraduate researcher at the University of Vilnova in Pennsylvania and author of an upcoming paper.

The magnetic field in the solar system cannot be measured directly unless it is isolated. So about 50 years ago, scientists were looking for a way to properly insert the magnetic field from the surface of the sun into the space of the planet, known in potential physics as extrapolation. Using observations of existing Sophia’s central magnetic fields, the team modified this method to estimate the magnetic field around 25,000 light-years around the cigarette galaxy.

“We can’t easily measure the magnetic field on this large scale, but we can do it in conjunction with helical physics,” said the scientist and lead author of the study at the Ames Sophia University Space Research Association. . “This new multidisciplinary approach gives us a great deal of insight into what constitutes stellar galaxies.”

Sophia is a joint project of NASA and the German Aerospace Center. NASA’s Ames Research Center in Silicon Valley, California, administers Sophia’s program, science, and missions in partnership with the Sofia Institute of Space Research at the University of Columbia, Maryland, and the University of Stuttgart. The aircraft is housed in the NASA Armstrong Flight Research Center Building 703 in Palladium, California. High-quality air-to-air train camera equipment developed by NASA Jet Proposition Laboratory and delivered to NASA.

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