43 citations
- Universidad Nacional Autónoma de MéxicoMX7 papers
- Centro de Investigación Científica y de Educación Superior de EnsenadaMX1 paper
- Cornell UniversityUS1 paper
- Gemini South ObservatoryCL1 paper
- Instituto de Astrofísica de AndalucíaES1 paper
- Instituto de Ciencia de Materiales de MadridES1 paper
- Johns Hopkins UniversityUS1 paper
- Leiden UniversityNL1 paper
- Lyon 1 UniversitéFR1 paper
- Max Planck Institute for AstronomyDE1 paper
- Observatoire de LyonFR1 paper
- Ollscoil na Gaillimhe – University of GalwayIE1 paper
7 papers
Tunnel spectroscopy in ac-driven quantum dot nanoresonators
J. Villavicencio, I. Maldonado, R. Sánchez +2
Electronic transport in a triple quantum dot shuttle device in the presence of an ac field is analyzed within a fully quantum mechanical framework. A generalized density matrix for…
Multiple and Precessing Collimated Outflows in the Planetary Nebula IC 4634
M. A. Guerrero, L. F. Miranda, A. Riera +6
With its remarkable double-S shape, IC 4634 is an archetype of point-symmetric planetary nebulae (PN). In this paper, we present a detailed study of this PN using archival HST WFPC…
A First Estimate Of The X-Ray Binary Frequency As A Function Of Star Cluster Mass In A Single Galactic System
D. M. Clark, S. S. Eikenberry, B. R. Brandl +7
We use the previously-identified 15 infrared star-cluster counterparts to X-ray point sources in the interacting galaxies NGC 4038/4039 (the Antennae) to study the relationship bet…
BF Eridani: a cataclysmic variable with a massive white dwarf and an evolved secondary
V. V. Neustroev, S. Zharikov
We present high- and medium-resolution spectroscopic observations of the cataclysmic variable BF Eri during its low and bright states. The orbital period of this system was found t…
Large Scale Flows from Orion-South
W. J. Henney, C. R. O'Dell, Luis A. Zapata +3
Multiple optical outflows are known to exist in the vicinity of the active star formation region called Orion-South (Orion-S). We have mapped the velocity of low ionization feature…
Relation between source and temperature fluctuations in photoionized nebulae
Luc Binette, Pierre Ferruit, Wolfgang Steffen +1
The magnitude of the temperature fluctuations (t^2) required to explain the observed inconsistencies between metallicities inferred from recombination lines and from forbidden line…