On the Geometry of the Near-Core Magnetic Field in Massive Stars
R. P. Ratnasingam et al 2024 ApJL 977 L30 Magnetohydrodynamic simulations of stellar interiors find unexpected behavior in stellar magnetic fields at the convective–radiative boundary, which has…
Read the full articleYou might also wanna read
Stellar Pulsations Shape Supernova Explosions: New research challenges the standard models of final moments of massive stars.
A new study published in The Astrophysical Journal Letters has found that the pulsations experience by red supergiant stars in the final sta
fys.kuleuven.be·2mo ago
Spectroscopic Classification of ASASSN-25cm as a Classical Nova
Original link submitted from IFL Science: Comments URL: Points: 12 # Comments: 1
astronomerstelegram.org·1y ago
Helioseismology Reveals Unexpected Changes in the Sun's 11-Year Magnetic Cycle
The Sun has a heartbeat. Every eleven years it swells with magnetic fury, hurling solar flares and charged particles into space, sparking au
universetoday.com·1mo ago
GRMHD simulations explore black hole accretion variability in X-ray binary transients
Black hole accretion must be SANE or MAD, right? Maybe not...read to learn more!
astrobites.org·29d ago
Comments
Sign in to join the conversation.
No comments yet. Be the first.