Powered by OpenAIRE graph
Found an issue? Give us feedback
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/ CONICET Digitalarrow_drop_down
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
CONICET Digital
Conference object . 2022
License: CC BY NC SA
Data sources: CONICET Digital
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
CONICET Digital
Article . 2022
License: CC BY NC SA
Data sources: CONICET Digital
image/svg+xml Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao Closed Access logo, derived from PLoS Open Access logo. This version with transparent background. http://commons.wikimedia.org/wiki/File:Closed_Access_logo_transparent.svg Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao
Servicio de Difusión de la Creación Intelectual
Article . 2022
Data sources: Servicio de Difusión de la Creación Intelectual
 View all 3 versions
Claim

Colliding winds in ultraluminous X-ray sources

descriptionPublicationkeyboard_double_arrow_right Article , Conference object 01 Jan 2022 Argentina English Publisher:Asociación Argentina de Astronomía.
Authors: Abaroa, Leandro; Romero, Gustavo Esteban; Sotomayor Checa, Pablo Omar;

handle: 11336/218607 , 11336/235500

Colliding winds in ultraluminous X-ray sources

Abstract

Ultraluminous X-ray sources (ULX) are objects with luminosities that exceed the Eddington limitfor a stellar-mass black hole. In these closed binary systems, the star overflows its Roche lobe and the black holeaccretes matter at a supercritical rate. The upper layers of the disk are no longer in equilibrium and are ejectedas a powerful radiation-driven wind that interacts with the wind from the star producing shocks where particlescan be accelerated up to relativistic energies and then cool down yielding a broadband spectrum

Fil: Sotomayor Checa, Pablo Omar. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina

Fil: Romero, Gustavo Esteban. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina

Fil: Abaroa, Leandro. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina

63º Reunión Anual de la Asociación Argentina de Astronomía

Instituto de Astronomía Teórica y Experimental

Observatorio Astronómico de Córdoba

Argentina

Córdoba

Country
Argentina
Related Organizations
Keywords

Ciencias Astronómicas, accretion, accretion disks, stars: winds, outflows, accretion disks, STARS: BLACK HOLES, radiation mechanisms: non-thermal, outflows, 520, X-rays: binaries, accretion, STARS: WINDS, stars: winds, RADIATION MECHANISMS: NONTHERMAL, ACCRETION DISKS, https://purl.org/becyt/ford/1.3, https://purl.org/becyt/ford/1, stars: black holes

  • BIP!
    Impact byBIP!
    selected citations
    These citations are derived from selected sources.
    This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    		 0
    popularity
    This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
    		 Average
    influence
    This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    		 Average
    impulse
    This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
    		 Average
Powered by OpenAIRE graph
Found an issue? Give us feedback
selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average
Green