Direct spectroscopic observation of matter falling onto a compact stellar object

GX 301-2 is an accreting x-ray pulsar with a massive hypergiant companion WRAY 977, embedded within a dense circumstellar environment. We report on detected redshifted hydrogen- and helium-like iron lines, together with transitions from lower ionization states, observed with XRISM/Resolve during an x-ray flare. Notably, these spectral features evolve from absorption lines at the beginning of the observation to emission lines at the end, with intervening phases exhibiting a mixture of both absorption and emission features. This behavior constitutes direct evidence of inflowing material accreting onto the neutron star. The results suggest a dynamic accretion geometry, evolving from predominantly radial inflow to a transverse, potentially disk-like configuration during the x-ray flare. Observations of inflowing matter thus constitute a direct test of accretion hypotheses and highlight the complex interplay between stellar wind and transient accretion disks in wind-accreting systems.

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Publication Details

Journal
Science Advances
Published
2026-09-18
DOI
https://doi.org/10.1126/sciadv.aef6686
Primary Topic
Astrophysical Phenomena and Observations
Type
article
Field-Weighted Citation Impact
0.00

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article

Direct spectroscopic observation of matter falling onto a compact stellar object

Ehud Behar, Pragati Pradhan, J. Wilms, Roi Rahin et al.
Science Advances
Astrophysical Phenomena and Observations
article

Direct spectroscopic observation of matter falling onto a compact stellar object

Ehud Behar, Pragati Pradhan, J. Wilms, Roi Rahin, M. Lorenz, Maurice A. Leutenegger, Natalie Hell, Joel B. Coley, Ralf Ballhausen, Nazma Islam, Tim Kallman, A. Zainab, Daisy Zamora
article en

Abstract

GX 301-2 is an accreting x-ray pulsar with a massive hypergiant companion WRAY 977, embedded within a dense circumstellar environment. We report on detected redshifted hydrogen- and helium-like iron lines, together with transitions from lower ionization states, observed with XRISM/Resolve during an x-ray flare. Notably, these spectral features evolve from absorption lines at the beginning of the observation to emission lines at the end, with intervening phases exhibiting a mixture of both absorption and emission features. This behavior constitutes direct evidence of inflowing material accreting onto the neutron star. The results suggest a dynamic accretion geometry, evolving from predominantly radial inflow to a transverse, potentially disk-like configuration during the x-ray flare. Observations of inflowing matter thus constitute a direct test of accretion hypotheses and highlight the complex interplay between stellar wind and transient accretion disks in wind-accreting systems.

Science AdvancesVol. 12(38)
Lawrence Livermore National Laboratory (US), Goddard Space Flight Center (US), Howard University (US), Manipal Academy of Higher Education (IN), Technion – Israel Institute of Technology (IL), Friedrich-Alexander-Universität Erlangen-Nürnberg (DE), United States Naval Academy (US), Deleted Institution, University of Maryland, College Park (US), University of Maryland, Baltimore County (US), Embry–Riddle Aeronautical University (US)
U.S. Department of Energy, National Aeronautics and Space Administration, Israel Science Foundation, National Aeronautics and Space Administration Postdoctoral Program
Openalex Percentile: Top 11%
Astrophysical Phenomena and Observations
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