Zobrazeno 1 - 10
of 43
pro vyhledávání: '"J Reyes-Iturbide"'
Autor:
J Reyes-Iturbide, I Ramírez-Ballinas, M Rosado, D Núñez, P Ambrocio-Cruz, L Arias, R Gabbasov
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 516:6055-6065
We present observations of the optical and X-ray emission from the Galactic supernova remnant W51C. From [S ii] Fabry–Pérot interferometry and H α and [S ii] images we detect filaments that are part of the optical counterpart of the supernova rem
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::16a90e0b3c4ca22790f87f0accad53f5
https://doi.org/10.1093/mnras/stac2568
https://doi.org/10.1093/mnras/stac2568
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 511:3420-3427
N70 is a giant superbubble (SB) produced by the stellar cluster LH 114. The dynamic of the stellar SB can be explained with hydrodynamic simulations. However, the explanation of the observed X-ray luminosity is still a matter of debate. Observations
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::05a845b194a2d3e8bfdf5d0bed815460
https://doi.org/10.1093/mnras/stac292
https://doi.org/10.1093/mnras/stac292
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 499:4213-4222
We present observations in X-ray and optical emission of the supernova remnant (SNR) 0520–69.4 in the Large Magellanic Cloud. Using XMM–Newton observatory data, we produced images of the diffuse X-ray emission and spectra to obtain the X-ray para
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::12c1ad5c092b965d4baf9729b82cf014
https://doi.org/10.1093/mnras/staa3138
https://doi.org/10.1093/mnras/staa3138
Autor:
E. Matias Schneiter, I. Ramírez-Ballinas, Margarita Rosado, J. Reyes-Iturbide, Pablo F. Velázquez
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
We present 3D hydrodynamical simulations of the circumstellar bubble from a Wolf-Rayet runaway star. In the models two properties were taken into account: (a) the proper motion of the central star through the interstellar medium (ISM) and (b) the evo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6ba4b5f42cc947f7b530c2bafab9e5c1
https://doi.org/10.22201/ia.01851101p.2019.55.02.09
https://doi.org/10.22201/ia.01851101p.2019.55.02.09
Akademický článek
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Autor:
J. Reyes-Iturbide, Martín A. Guerrero, Wei Sun, You-Hua Chu, John S. Gallagher, Vincent Hénault-Brunet, L. M. Oskinova, Robert A. Gruendl, Chris Evans
SXP 1062 is an exceptional case of a young neutron star in a wind-fed high-mass X-ray binary associated with a supernova remnant. A unique combination of measured spin period, its derivative, luminosity and young age makes this source a key probe for
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b1de99ccc09f70dc0e21278086efe019
We present a study of the diffuse X-ray emission from the star forming region LMC-N 57 in the Large Magellanic Cloud (LMC). We use archival XMM-Newton observations to unveil in detail the distribution of hot bubbles in this complex. X-ray emission is
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f9de7eb3a0ef15057411279b364b04d1
Autor:
Martín A. Guerrero, Robert A. Gruendl, Lidia M. Oskinova, John S. Gallagher, J. Reyes-Iturbide, W. Sun, Chris Evans, Vincent Hénault-Brunet, You-Hua Chu
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 420:L13-L17
We report on a new Be/X-ray pulsar binary located in the Wing of the Small Magellanic Cloud (SMC). The strong pulsed X-ray source was discovered with the Chandra and XMM- Newton X-ray observatories. The X-ray pulse period of 1062 s is consistently de
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ad42e59fdb8fc01a85eaea5e36c527c4
https://doi.org/10.1111/j.1745-3933.2011.01183.x
https://doi.org/10.1111/j.1745-3933.2011.01183.x
Autor:
J. C. Toledo-Roy, E. M. Reynoso, Ricardo F. González, F. De Colle, J. Reyes-Iturbide, Stan Kurtz, Pablo F. Velázquez
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 395:351-357
We present a two-component supernova remnant model for the case of Magellanic remnant DEM L316 obtained from two-dimensional, axisymmetric hydrodynamic simulations. We study different scenarios which consider a possible collision between the shells a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6d05ae302bd2a5df0a355614d2593543
https://doi.org/10.1111/j.1365-2966.2009.14517.x
https://doi.org/10.1111/j.1365-2966.2009.14517.x
Autor:
Margarita Rosado, Ary Rodríguez-González, J. Reyes-Iturbide, Pablo F. Velázquez, Ricardo F. González, Alejandro Esquivel
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 394:1009-1015
We present 3D hydrodynamical simulations of the superbubble M17, also known as the Omega nebula, carried out with the adaptive grid code yguazu'-a, which includes radiative cooling. The superbubble is modelled considering the winds of 11 individual s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::70361125b4c205ac72813da4913aede6
https://doi.org/10.1111/j.1365-2966.2008.14386.x
https://doi.org/10.1111/j.1365-2966.2008.14386.x