Category Astronomy/Space

First-ever Detection of a Mid-Infrared Flare in SagittariusA*, the Milky Way’s supermassive black hole

Using the MIRI instrument onboard the James Webb Space Telescope, an international team of scientists made the first-ever detection of a mid-IR flare from Sagittarius A*, the supermassive blackhole at the heart of the Milky Way. In simultaneous radio observations, the team found a radio counterpart of the flare lagging behind in time. The paper is published on the arXiv preprint server.

Scientists have been actively observing Sagittarius A* (Sgr A)—a supermassive black hole roughly 4 million times the mass of the sun— since the early 1990s. Sgr A regularly exhibits flares that can be observed in multiple wavelengths, allowing scientists to see different views of the same flare and better understand how it emits light and how the emission is generated...

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‘What is that?’ Scientists explain White Patch that appears Near Northern Lights

Images of the aurora borealis showing the structured continuum emission.Courtesy Faculty of Science research team

A whitish, gray patch that sometimes appears in the night sky alongside the northern lights has been explained for the first time by researchers at the University of Calgary.

The article, which was published on Dec. 30 in the journal Nature Communications, explores a “structured continuum emission” that’s associated with aurora borealis.

“You’d see this dynamic green aurora, you’d see some of the red aurora in the background and, all of a sudden, you’d see this structured—almost like a patch—gray-toned or white toned-emission connected to the aurora,” says Dr. Emma Spanswick, Ph.D...

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High-Resolution Simulations Explore the Physics of Star Formation

Rocking the magnetic cradle of stellar birth
The new simulations show a cross section of the star and its surrounding disk of gas. In the left image, where the young star is weakly magnetized, gas can be seen flowing freely from the surrounding disk of material to the surface of the protostar. In the right image, material flows along the magnetic field lines towards the star’s poles, in a much more defined flow. Credit: Astronomy & Astrophysics (2024). DOI: 10.1051/0004-6361/202451842

Stars are born in clouds of gas and dust, making it difficult to observe their early development. But researchers at Chalmers have now succeeded in simulating how a star with the mass of the sun absorbs material from the surrounding disk of material—a process called accretion.

The researchers simulated four stars with the same mass but with v...

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Helical Magnetic Fields: A Universal Mechanism for Jet Collimation?

Results of the Rotation Measure analysis in the HH80-81 jet. The left image shows the streamline image of the component of the magnetic field parallel to the plane of the sky. In the middle panel, the color scale of the RM indicates the direction of the magnetic field along the line of sight, i.e., red, away from the observer, and blue, towards the observer. The right panel shows a scheme depicting the 3D configuration of the magnetic field, exhibiting a helical topology.
Credit: Rodríguez-Kamenetzky et al. 2025, The Astrophysical Journal.

New observations from the National Science Foundation National Radio Astronomy Observatory’s (NSF NRAO) Karl G...

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