Unveiling the nature ultra-luminous X-ray sources through the kinematics and structure of their optical counterpart

Fuentes-Carrera I.; Salinas A.; Rosado M.; Moreno-Méndez E.; Arias L.; Repetto P.; Borissova J.; Gonçalves D. R.; Flores H.

Vol. 44 No. 1 (2014), Contributions

Vol. 44 No. 1 (2014)

Contributions

Unveiling the nature ultra-luminous X-ray sources through the kinematics and structure of their optical counterpart

Fuentes-Carrera I.⁺⁻
Salinas A.⁺⁻
Rosado M.⁺⁻
Moreno-Méndez E.⁺⁻
Arias L.⁺⁻
Repetto P.⁺⁻
Borissova J.⁺⁻
Gonçalves D. R.⁺⁻
Flores H.⁺⁻

Fuentes-Carrera I.

Escuela Superior de Física y Matemáticas, Instituto Politécnico Nacional, U.P. Adolfo López Mateos, Zacatenco 07730 México D.F., México

Salinas A.

Escuela Superior de Física y Matemáticas, Instituto Politécnico Nacional, U.P. Adolfo López Mateos, Zacatenco 07730 México D.F., México

Rosado M.

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Moreno-Méndez E.

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Arias L.

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Repetto P.

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Borissova J.

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Gonçalves D. R.

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Flores H.

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Keywords

X-rays: Galaxies
Stars: Black Holes
ISM: Kinematics and Dynamics
ISM: Jets and outflows

How to Cite

Unveiling the nature ultra-luminous X-ray sources through the kinematics and structure of their optical counterpart. (2014). Revista Mexicana De Astrofísica Y Astronomía Serie De Conferencias, 44(1), 110-110. https://astronomia.unam.mx/journals/rmxac/article/view/2014rmxac..44..110f

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Abstract

We present observations scanning Fabry-Perot observations of the nearby galaxy NGC 5402 hosting one bright ultra-luminous X-ray source as part of a project to study the kinematics of the extended counterpart of this ULX and nature of the ionization of the gas.

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Unveiling the nature ultra-luminous X-ray sources through the kinematics and structure of their optical counterpart

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