activity
19972025
most citedAnatomy of the hyper-runaway star LP 40-365 with Gaia

44 citations · 209 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.SR2025★ 7 cited

Testing the mass-radius relation of white dwarfs in common proper motion pairs I.Hydrogen-dominated atmospheres

Roberto Raddi, Alberto Rebassa-Mansergas, Santiago Torres +6

The main goal of this work was to measure the masses and radii of white dwarfs that belong to widely separated, common proper motion binaries with non-degenerate companions. These…

astro-ph.SR2019★ 13 cited

Full inversion of solar relativistic electron events measured by the Helios spacecraft

Daniel Pacheco, Neus Agueda, Angels Aran +3

Up to present, the largest data set of SEP events in the inner heliosphere are the observations by the two Helios spacecraft. We re-visit a sample of 15 solar relativistic electron…

astro-ph.SR2018★ 44 cited

Anatomy of the hyper-runaway star LP 40-365 with Gaia

R. Raddi, M. A. Hollands, B. T. Gaensicke +4

LP 40-365 (aka GD 492) is a nearby low-luminosity hyper-runaway star with an extremely unusual atmospheric composition, which has been proposed as the remnant of a white dwarf that…

astro-ph.SR2018★ 38 cited

Further insight on the hypervelocity white dwarf, LP 40-365 (GD 492): a nearby emissary from a single-degenerate Type Ia supernova

R. Raddi, M. A. Hollands, D. Koester +4

The recently discovered hypervelocity white dwarf LP 40-65 (aka GD 492) has been suggested as the outcome of the failed disruption of a white dwarf in a sub-luminous Type Ia supern…

astro-ph.SR2017★ 14 cited

Spread of the dust temperature distribution in circumstellar disks

S. Heese, S. Wolf, A. Dutrey +1

Accurate temperature calculations for circumstellar disks are particularly important for their chemical evolution. Their temperature distribution is determined by the optical prope…

astro-ph.SR2014★ 16 cited

How dusty is alpha Centauri? Excess or non-excess over the infrared photospheres of main-sequence stars

J. Wiegert, R. Liseau, P. Thébault +19

[Abridged] Debris discs around main-sequence stars indicate the presence of larger rocky bodies. The components of the nearby binary aCentauri have higher than solar metallicities,…