A NuSTAR Study of Quasiperiodic Oscillations from the Ultraluminous X-Ray Sources in M82

Abstract The study of quasiperiodic oscillations (QPOs) in X-ray binaries provides valuable insights into the physics of accretion around compact objects. The M82 galaxy hosts multiple ultraluminous X-ray sources, including two prominent ones—X-1 and X-2—where X-1 is suspected to harbor an intermediate-mass black hole. In this work, we analyze data from 39 NuSTAR observations acquired between 2014 and 2024 to investigate the aperiodic X-ray variability in M82. In particular, we study in detail the evolution of the QPOs from M82 X-1 in the range 20–300 mHz. We do not find additional timing features in the data, besides a frequently present broad noise component at lower frequencies. The QPO behaves similarly to other classes of low-frequency oscillations in accreting compact objects, both black holes and neutron stars.

Authors

Institutions

Publication Details

Journal
The Astrophysical Journal
Published
2025-08-18
DOI
https://doi.org/10.3847/1538-4357/aded8a
Citations
2
Primary Topic
Astrophysical Phenomena and Observations
Type
article
Field-Weighted Citation Impact
2.31

Funders

Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

A NuSTAR Study of Quasiperiodic Oscillations from the Ultraluminous X-Ray Sources in M82

Murray Brightman, M. Pilia, M. Imbrogno, D. J. Walton et al.
2 citations
The Astrophysical Journal
Astrophysical Phenomena and Observations
2.31
article

A NuSTAR Study of Quasiperiodic Oscillations from the Ultraluminous X-Ray Sources in M82

Murray Brightman, M. Pilia, M. Imbrogno, D. J. Walton, Thomas J. Maccarone, Silvia Columbu, F. Fuerst, Karl Förster, Matthew Middleton, Eleonora Veronica Lai, Hannah P. Earnshaw, Marianne Heida, Brian W. Grefenstette, G. Rodríguez, Matteo Bachetti, Hamza El Byad
article en
2 citations

Abstract

Abstract The study of quasiperiodic oscillations (QPOs) in X-ray binaries provides valuable insights into the physics of accretion around compact objects. The M82 galaxy hosts multiple ultraluminous X-ray sources, including two prominent ones—X-1 and X-2—where X-1 is suspected to harbor an intermediate-mass black hole. In this work, we analyze data from 39 NuSTAR observations acquired between 2014 and 2024 to investigate the aperiodic X-ray variability in M82. In particular, we study in detail the evolution of the QPOs from M82 X-1 in the range 20–300 mHz. We do not find additional timing features in the data, besides a frequently present broad noise component at lower frequencies. The QPO behaves similarly to other classes of low-frequency oscillations in accreting compact objects, both black holes and neutron stars.

The Astrophysical JournalVol. 989(2)
Texas Tech University (US), University of Hertfordshire (GB), University of Cagliari (IT), Astronomical Observatory of Rome (IT), European Space Astronomy Centre (ES), Osservatorio Astronomico di Cagliari (IT), University of Southampton (GB), National Institute for Astrophysics (IT)
European Commission, Science and Technology Facilities Council
Openalex Percentile: Top 11%
Astrophysical Phenomena and Observations
2.31
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.