Multi-Observatory Research of Young Stellar Energetic Flares (MORYSEF): X-Ray-flare-related Phenomena and Multi-epoch Behavior

• Published in: The Astrophysical journal Vol. 976; no. 2; pp. 195 - 217
• Main Authors: Getman, Konstantin V., Feigelson, Eric D., Waggoner, Abygail R., Cleeves, L. Ilsedore, Forbrich, Jan, Ninan, Joe P., Kochukhov, Oleg, Airapetian, Vladimir S., Dzib, Sergio A., Law, Charles J., Rab, Christian
• Format: Journal Article
• Language: English
• Published: Philadelphia The American Astronomical Society 01.12.2024; IOP Publishing
• Subjects: Arrays; Circumstellar habitable zone; Emission; Ionization; Irradiation; Magnetic fields; Magnetic properties; Observatories; Orion nebula; Planet formation; Pre-main sequence stars; Protoplanetary disks; Radio telescopes; Stars; Stellar flares; Stellar magnetic fields; Stellar mass; Stellar surfaces; Stellar x-ray flares; Very Long Baseline Array (VLBA); X-ray emissions; X-ray stars; X-rays

The most powerful stellar flares driven by magnetic energy occur during the early pre-main-sequence (PMS) phase. The Orion Nebula represents the nearest region populated by young stars, showing the greatest number of flares accessible to a single pointing of Chandra. This study is part of a multi-ob...