Skip to main content

AI Bias Analysis

4 models · Takes ~15 seconds

Phys.org

Tandem superflare observations reveal origin of the stellar Fe Kα line

Tandem superflare observations reveal origin of the stellar Fe Kα line
ShareXFacebook

The Fe Kα line, or iron Kα line, is often used in astronomical research to understand the physical composition of astronomical objects. This line is produced when a K-shell electron of an iron ion in the photosphere—the gas on the stellar surface—is ejected by an external process, and has been detected in X-ray spectra of solar and stellar flares. Yet the dominant mechanism behind this ionization

P

Source

Phys.org

Read full article at Phys.org

Opens original article in a new tab

Advertisement

Related Science Stories

The planet haul that changes everything
Phys.org

The planet haul that changes everything

Finding planets used to be a painstaking business. Astronomers would fix their gaze on a handful of carefully chosen stars, watch and wait, and hope to catch the faint dip in starlight that signals a world passing in front of its host. It worked. It worked brilliantly. But it also meant we were fishing with a very small net in a very big ocean.

Read more →
Advertisement