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19992020
most citedDo instabilities in high-multiplicity systems explain the existence of close-in white dwarf planets?

35 citations · 138 across the 15 of their papers we have counts for

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6 papers · 1 filter

astro-ph.SR20201 cited

Synthetic spectroscopic indices for identifying multiple stellar populations in globular clusters

Emanuele Bertone, Miguel Chávez, J. César Mendoza

We present an investigation of synthetic spectroscopic indices that can plausibly help in identifying the presence of multiple stellar populations in globular clusters. The study i…

astro-ph.SR2018

Wandering near the red edge: photometric observations of three cool ZZ Ceti stars

Zs. Bognár, M. Paparó, Á. Sódor +11

We summarize our findings on three cool ZZ Ceti type pulsating white dwarfs. We determined eight independent modes in HS 0733+4119, of which seven are new findings. For GD 154, we…

astro-ph.SR20176 cited

Asteroseismology of the ZZ Ceti star KUV 08368+4026

C. Li, J. -N. Fu, G. Vauclair +5

Asteroseismology is a unique tool to explore the internal structure of stars through both observational and theoretical research. The internal structure of pulsating hydrogen shell…

astro-ph.SR20175 cited

Infrared excesses in stars with and without planets using revised photometry

Raul F. Maldonado, Miguel Chavez, Emanuele Bertone +1

We present an analysis on the potential prevalence of mid infrared excesses in stars with and without planetary companions. Based on an extended database of stars detected with the…

astro-ph.SR20172 cited

Mg, Al, Si, Ca, Ti, Fe, and Ni abundance for a sample of solar analogues

Ricardo López-Valdivia, Emanuele Bertone, Miguel Chávez

We report on the determination of chemical abundances of 38 solar analogues, including 11 objects previously identified as super metal-rich stars. We have measured the equivalent w…

astro-ph.SR201513 cited

Lithium abundance in a sample of solar-like stars

R. López-Valdivia, J. B. Hernández-Águila, E. Bertone +3

We report on the determination of the lithium abundance [A(Li)] of 52 solar-like stars. For 41 objects the A(Li) here presented corresponds to the first measurement. We have measur…