output
20152024
most citedAtomic data for the Gaia-ESO Survey

186 citations

Showing 2022Show all

25 papers · 1 filter

astro-ph.SR202220 cited

The White Dwarf Binary Pathways Survey -- IX. Three long period white dwarf plus subgiant binaries

S. G. Parsons, M. S. Hernandez, O. Toloza +8

Virtually all binaries consisting of a white dwarf with a non-degenerate companion can be classified as either close post-interaction systems (with orbital periods of a few days or…

astro-ph.SR202254 cited

white dwarfs within 40 pc III: spectroscopic observations of new candidates in the southern hemisphere

Mairi W. O'Brien, P. -E. Tremblay, N. P. Gentile Fusillo +31

We present a spectroscopic survey of 248 white dwarf candidates within 40 pc of the Sun; of these 244 are in the southern hemisphere. Observations were performed mostly with the Ve…

astro-ph.EP202216 cited

A kinematic excess in the annular gap and gas depleted cavity in the disc around HD 169142

Himanshi Garg, Christophe Pinte, Iain Hammond +6

We present ALMA band 6 images of the 12CO, 13CO and C18O J=2-1 line emissions for the circumstellar disc around HD 169142, at ~8 au spatial resolution. We resolve a central gas dep…

astro-ph.SR20224 cited

Infrared variability of young solar analogs in the Lagoon Nebula

C. Ordenes-Huanca, M. Zoccali, A. Bayo +9

T Tauri stars are low-mass pre-main sequence stars that are intrinsically variable. Due to the intense magnetic fields they possess, they develop dark spots on their surface that,…

astro-ph.SR202232 cited

The White Dwarf Binary Pathways Survey -- VIII: a post common envelope binary with a massive white dwarf and an active G-type secondary star

M. S. Hernandez, M. R. Schreiber, S. G. Parsons +6

The white dwarf binary pathways survey is dedicated to studying the origin and evolution of binaries containing a white dwarf and an intermediate-mass secondary star of the spectra…

astro-ph.SR202218 cited

Physical properties of accretion shocks toward the Class I protostellar system Oph-IRS 44

E. Artur de la Villarmois, V. V. Guzmán, J. K. Jørgensen +6

(Abridged) Physical processes such as accretion shocks are thought to be common in the protostellar phase, where the envelope component is still present, and they can release molec…