Sara Elisa Motta

University of Oxford

United Kingdom

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Articles (17)

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2025

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2023

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2023

Collaborators (11)

Mariano Méndez

University of Groningen

NETHERLANDS

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A K Hughes

University of Alberta

CANADA

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Adam Ingram

Lecturer and Royal Society URF

Newcastle University

UNITED KINGDOM

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Jorge Casares

Professor

Instituto de Astrofísica de Andalucía

SPAIN

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James Miller-Jones

Professor

Curtin University

AUSTRALIA

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Darin Ragozzine

Professor

Brigham Young University

UNITED STATES

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Montserrat Armas Padilla

Instituto de Astrofísica de Andalucía

SPAIN

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Paolo Esposito

Università degli Studi di Pavia

ITALY

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David Russell

New York University

UNITED STATES

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Francesco Carotenuto

University of Oxford

UNITED KINGDOM

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Dominic Walton

University of Hertfordshire

UNITED KINGDOM

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Sara Elisa Motta

Research Interests

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Articles (17)

The connection between the fastest astrophysical jets and the spin axis of their black hole

MeerKAT discovers a jet-driven bow shock near GRS 1915+105

Quantifying jet–interstellar medium interactions in Cyg X-1: Insights from dual-frequency bow shock detection with MeerKAT

Type I X-ray burst emission reflected into the eclipses of EXO 0748−676

A new pulsating neutron star in the ultraluminous X-ray source NGC 4559 X7?

Multi-band study of the flaring mode emission in the transitional millisecond pulsar PSR J1023+0038

Peculiar radio-bright behaviour of the Galactic black hole transient 4U 1543−47 in the 2021–2023 outburst

The restless population of bright X-ray sources of NGC 3621

Swift J1727.8–1613 Has the Largest Resolved Continuous Jet Ever Seen in an X-Ray Binary

Skipping a beat: Discovery of persistent quasi-periodic oscillations associated with pulsed fraction drop of the spin signal in M51 ULX-7

Radio observations of the 2022 outburst of the transitional Z-Atoll source XTE J1701−462

Particle acceleration at the bow shock of runaway star LS 2355: non-thermal radio emission but no γ-ray counterpart

Rethinking the 67 Hz QPO in GRS 1915+105: Type C quasi-periodic oscillations at the innermost stable circular orbit

A possible third body in the X-ray system GRS 1747−312 and models with higher order multiplicity

Highly Significant Detection of X-Ray Polarization from the Brightest Accreting Neutron Star Sco X-1

Fast infrared winds during the radio-loud and X-ray obscured stages of the black hole transient GRS 1915+105

A systematic study of the high-frequency bump in the black-hole low-mass X-ray binary GX 339 − 4

Collaborators (11)

Mariano Méndez

A K Hughes

Adam Ingram

Jorge Casares

James Miller-Jones

Darin Ragozzine

Montserrat Armas Padilla

Paolo Esposito

David Russell

Francesco Carotenuto

Dominic Walton

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