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20012020
most citedUnderstanding the origin of white dwarf atmospheric pollution by dynamical simulations based on detected three-planet systems

31 citations · 41 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.EP2020★ 31 cited

Understanding the origin of white dwarf atmospheric pollution by dynamical simulations based on detected three-planet systems

R. F. Maldonado, E. Villaver, A. J. Mustill +2

Between 25-50 % of white dwarfs (WD) present atmospheric pollution by metals, mainly by rocky material, which has been detected as gas/dust discs, or in the form of photometric tra…

astro-ph.SR2016★ 6 cited

ALMA's view of the Sun's nearest neighbours: The submm/mm SEDs of the alpha Centauri binary and a new source

R. Liseau, V. De la Luz, E. O'Gorman +3

The precise mechanisms that provide the non-radiative energy for heating the chromosphere and the corona of the Sun and other stars are at the focus of intense contemporary researc…

astro-ph.SR2015

A new submm source within a few arcseconds of Centauri: ALMA discovers the most distant object of the solar system

R. Liseau, W. Vlemmings, E. O'Gorman +3

We recently announced the detection of an unknown submillimeter source in our ALMA observations of alpha Cen AB. The source was detected in two epochs, a strong detection at 445~GH…

astro-ph.SR2009★ 4 cited

Snapshot metallicity estimate of resolved stellar systems through Lick Fe5270 diagnostic

Alberto Buzzoni, Emanuele Bertone, Miguel Chavez

We outline a new method to derive a "snapshot" metallicity estimate of stellar systems (providing one resolves at least the brightest part of the CMD) just on the basis of low-reso…

astro-ph2001

Multiwavelenght analysis of Gl 355 (LQ Hya)

S. Covino, G. Tagliaferri, E. Bertone +8

We discuss ROSAT, ASCA, {\it Beppo}SAX and optical observations of the young active star Gl 355. During the ROSAT observation a strong flare was detected with a peak flux more than…

astro-ph2001

A Grid of Synthetic Stellar UV Fluxes

Lino H. Rodriguez-Merino, Miguel Chavez, Alberto Buzzoni +1

We present preliminary results of a large project aimed at creating an extended theoretical and observational database of stellar spectra in the ultraviolet wavelength range. This…