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

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...

Fuld beskrivelse

Bibliografiske detaljer

Principais autores:	Konstantin V. Getman, Eric D. Feigelson, Abygail R. Waggoner, L. Ilsedore Cleeves, Jan Forbrich, Joe P. Ninan, Oleg Kochukhov, Vladimir S. Airapetian, Sergio A. Dzib, Charles J. Law, Christian Rab
Format:	Artigo
Sprog:	Inglês
Udgivet:	IOP Publishing 2024-01-01
Serier:	The Astrophysical Journal
Fag:	Pre-main sequence stars X-ray stars Stellar magnetic fields Stellar x-ray flares Stellar flares Protoplanetary disks
Online adgang:	https://doi.org/10.3847/1538-4357/ad8562
Tags:	Tilføj Tag Ingen Tags, Vær først til at tagge denne postø!