activity
20092026
most citedDiscovery of millihertz quasi-periodic oscillations in the X-ray binary EXO 0748--676

23 citations · 68 across the 11 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

11 papers · 1 filter

astro-ph.HE2026

A cooler look at the environment of Cygnus X-1: Searching for dynamical interactions within cold molecular gas

Pau Bosch-Cabot, Alexandra J. Tetarenko, Valentí Bosch-Ramon +7

We present IRAM--30m observations aimed at identifying potential outflow-interstellar medium interaction sites in the vicinity of the black hole X-ray binary Cygnus X--1, which dis…

astro-ph.HE2026★ 1 cited

Optical outburst evolution of the transient black hole X-ray binary Swift J1727.8-1613: Disc response to jet ejections and late-outburst emergence of powerful disc winds

N. Castro Segura, K. Solomons, J. M. Corral-Santana +22

Swift J1727.81613 is a newly discovered transient low-mass X-ray binary harbouring a stellar-mass () black hole. We present state-resolved VLT/X-Shooter optical…

astro-ph.HE2025★ 5 cited

Chlorine and Potassium Enrichment in the Cassiopeia A Supernova Remnant

XRISM collaboration

The elements in the universe are synthesized primarily in stars and supernovae, where nuclear fusion favors the production of even-Z elements. In contrast, odd-Z elements are less…

astro-ph.HE2025

XRISM Observations of Accretion Disk Corona in Cyg X-2

Misaki Mizumoto, Hiromitsu Takahashi, Ehud Behar +6

We present the high-resolution X-ray spectrum of the Z-source Cygnus X-2, obtained with X-Ray Imaging and Spectroscopy Mission (XRISM). The observations have enabled a precise char…

astro-ph.HE2025

The Feasibility of Using Fe XXIII Metastable Transitions as a Density Diagnostic for LMXB Disk Winds

D. L. Moutard, L. R. Corrales, R. Tomaru +6

Low mass X-ray binaries (LMXBs) occasionally show signs of outflowing material from the accretion disk. Studying these outflows can inform the understanding of the geometry of the…

astro-ph.HE2024

Overionized plasma in the supernova remnant Sagittarius A East anchored by XRISM observations

XRISM Collaboration

Sagittarius A East is a supernova remnant with a unique surrounding environment, as it is located in the immediate vicinity of the supermassive black hole at the Galactic center, S…

astro-ph.HE2020★ 18 cited

Discovery of a thermonuclear Type I X-ray burst in infrared: new limits on the orbital period of 4U 1728-34

F. M. Vincentelli, Y. Cavecchi, P. Casella +4

We report the detection of an infrared burst lagging a thermonuclear Type I X-ray burst from the accreting neutron star 4U 1728-34 (GX 354-0). Observations were performed simultane…

astro-ph.HE2019★ 23 cited

Discovery of millihertz quasi-periodic oscillations in the X-ray binary EXO 0748--676

G. C. Mancuso, D. Altamirano, F. García +5

We report the discovery of millihertz quasi-periodic oscillations (mHz QPOs) from the bursting, high-inclination atoll neutron-star low-mass X-ray binary (NS LMXB) EXO 0748--676 wi…

astro-ph.HE2017★ 10 cited

The cooling, mass and radius of the neutron star in EXO 0748-676 in quiescence with XMM-Newton

Zheng Cheng, Mariano Mendez, Maria Diaz-Trigo +1

We analyse four XMM-Newton observations of the neutron-star low-mass X-ray binary EXO 0748676 in quiescence. We fit the spectra with an absorbed neutron-star atmosphere model, w…

astro-ph.HE2015★ 11 cited

Systematic Uncertainties in the Spectroscopic Measurements of Neutron-Star Masses and Radii from Thermonuclear X-ray Bursts. III. Absolute Flux Calibration

Tolga Guver, Feryal Ozel, Herman Marshall +3

Many techniques for measuring neutron star radii rely on absolute flux measurements in the X-rays. As a result, one of the fundamental uncertainties in these spectroscopic measurem…

astro-ph.HE2009

Distribution and Structure of Matter in and around Galaxies

Norbert S. Schulz, Glenn Allen, Mark W. Bautz +24

Understanding the origins and distribution of matter in the Universe is one of the most important quests in physics and astronomy. Themes range from astro-particle physics to chemi…