Search Publications

X-ray Observations of the Very-Faint X-ray Transient XMMSL1 J171900.4-353217: A New Candidate Neutron Star Low-Mass X-ray Binary
DOI: 10.48550/arXiv.2409.19649 Bibcode: 2024RMxAA..60..403A

Degenaar, N.; Wijnands, R.; Armas Padilla, M. +1 more

XMMSL1 J171900.4–353217 is a very-faint X-ray transient that was discovered in 2010 March when it exhibited an outburst. We report on 7 observations, obtained with the X-Ray Telescope (XRT) aboard the Neil Gehrels Swift Observatory between 2010 May and October. By fitting a single absorbed power-law model to the XRT spectra, we infer power-law ind…

2024 Revista Mexicana de Astronomia y Astrofisica
INTEGRAL XMM-Newton 0
X-ray Analysis of Seyfert 1 Galaxies with Optical Polarization: A Test for Unification Models
DOI: 10.48550/arXiv.2403.13194 Bibcode: 2024RMxAA..60..241G

Guainazzi, M.; Jiménez-Bailón, E.; Longinotti, A. L. +3 more

In accordance with the AGN Unified Model, observed polarization can be related to the orientation of the line of sight with respect to the torus. AGN X-ray emission arises from the central region and carries the imprints of the obscuring material. We aim to test a unified scheme based on optical polarization using X-ray absorption. Using the XMM-N…

2024 Revista Mexicana de Astronomia y Astrofisica
XMM-Newton 0
Tracing the Assembly Histories of Galaxy Clusters in the Nearby Universe
DOI: 10.22201/ia.01851101p.2023.59.02.13 Bibcode: 2023RMxAA..59..345C

Andernach, H.; Caretta, C. A.; Coziol, R. +10 more

We have compiled a sample of 67 nearby (z < 0.15) clusters of galaxies, for which on average more than 150 spectroscopic members are available and, by applying different methods to detect substructures in their galaxy distribution, we have studied their assembly history. Our analysis confirms that substructures are present in 70% of our sample,…

2023 Revista Mexicana de Astronomia y Astrofisica
XMM-Newton 1
The 2017 Release Cloudy
DOI: 10.48550/arXiv.1705.10877 Bibcode: 2017RMxAA..53..385F

Abel, N. P.; Keenan, F. P.; Ferland, G. J. +8 more

We describe the 2017 release of the spectral synthesis code Cloudy, summarizing the many improvements to the scope and accuracy of the physics which have been made since the previous release. Exporting the atomic data into external data files has enabled many new large datasets to be incorporated into the code. The use of the complete datasets is …

2017 Revista Mexicana de Astronomia y Astrofisica
XMM-Newton 1377
Radio Sources Embedded in the Dense Core B59, the ``Mouthpiece'' of the Pipe Nebula
DOI: 10.48550/arXiv.1308.2621 Bibcode: 2013RMxAA..49..345D

Loinard, L.; Rodríguez, L. F.; Dzib, S. A. +1 more

We present Very Large Array continuum observations made at 8.3 GHz toward the dense core B59, in the Pipe Nebula. We detect six compact sources, of which five are associated with the five most luminous sources at 70 µm in the region, while the remaining one is probably a background source. We propose that the radio emission is free-free from…

2013 Revista Mexicana de Astronomia y Astrofisica
XMM-Newton 7