activity
20032022
most citedNanodiamond dust and the far-ultraviolet quasar break

23 citations · 81 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.GA2022★ 1 cited

Optimized Spectral Energy Distribution for Seyfert Galaxies

Luc Binette, Yair Krongold, Sinhue A. R. Haro-Corzo +2

The temperature predicted by photoionization models for the Narrow Line Region of Seyfert 2 galaxies is lower than the value inferred from the observed [O III] λ4363A/λ5007A line r…

astro-ph.GA2020★ 17 cited

Active galactic nuclei ghosts: A systematic search for faded nuclei

Donaji Esparza-Arredondo, Natalia Osorio-Clavijo, Omaira González-Martín +5

Physical processes such as re-ignition, enhancement, and fading of active galactic nuclei (AGN) are not entirely understood because the timeline of these events is expected to last…

astro-ph.EP2018

Lightcurves for asteroids 18301 Konyukhov and 2022 West

Sinhué A. R. Haro-Corzo, Luis A. Villegas, Lorenzo Olguín +7

We report photometric analysis of two main-belt asteroids observed at the Observatorio Astronomico Nacional in the Sierra San Pedro Martir, Baja California, México. For 18301 Konyu…

astro-ph.SR2009★ 9 cited

Shaping point- and mirror-symmetric proto-planetary nebulae by the orbital motion of the central binary system

Sinhue A. R. Haro-Corzo, Pablo F. Velazquez, Alejandro C. Raga +2

We present 3D hydrodynamical simulations of a jet launched from the secondary star of a binary system inside a proto-planetary nebula. The secondary star moves around the primary i…

astro-ph2008

The big blue bump and soft X-ray excess of individual quasars

Sinhue A. R. Haro-Corzo, Luc Binette, Yair Krongold

For 11 quasar, we find that the soft X-ray excess component is not prolongation of the Big Blue Bump. Furthermore, adopting a theoretical continuum that is absorbed by the appropri…

astro-ph2007★ 4 cited

Quasar 3C298: a test-case for meteoritic nanodiamond 3.5 microns emission

J. A. de Diego, L. Binette, P. Ogle +3

We calculate the dust emission expected at 3.43 and 3.53 microns if meteoritic (i.e. hydrogenated) nanodiamonds are responsible for most of the far-UV break observed in quasars. We…