Evidence for Millihertz Oscillations in the bright atoll source GX 3+1
Malu Sudha, Renee M. Ludlam, Diego Altamirano, Edward M. Cackett, Mason Ng
astro-ph.HE
Submitted: 2026-06-30
Comments: Accepted for publication in ApJ
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Thermonuclear Burning on Rapidly Accreting Neutron Stars
- A Python Code for the Emmanoulopoulos et al. [arXiv:1305.0304] Light Curve Simulation Algorithm
- The first radius-expansion X-ray burst from GX 3+1
- Coronal Vertical Structure Variations in Normal Branch of GX 17+2 : AstroSa\v{t}s SXT and LAXPC perspective
Related papers
- Accreting Neutron Stars in Low-Mass X-ray Binaries
- Numerical Studies of Accretion Flows onto a Neutron Star Engulfed in a Massive Star
- Early panchromatic spectra reveal helium in the thermonuclear supernova 2024kce
- Multiwavelength Classification of Chandra Sources in Omega Centauri
- Impact of the equation of state on core collapse supernovae I: the low- T/W instability
- Secular Evolution of Quasiperiodic Eruptions: eRO-QPE2