activity
20162020
most citedExocomet signatures around the A-shell star Leo?

35 citations · 35 across the 1 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2020

The White Dwarf Binary Pathways Survey III: contamination from hierarchical triples containing a white dwarf

F. Lagos, M. R. Schreiber, S. G. Parsons +12

The White Dwarf Binary Pathways Survey aims at increasing the number of known detached A, F, G and K main sequence stars in close orbits with white dwarf companions (WD+AFGK binari…

astro-ph.SR2019

HR 10: A main-sequence binary with circumstellar envelopes around both components. Discovery and analysis

B. Montesinos, C. Eiroa, J. Lillo-Box +16

This paper is framed within a large project devoted to studying the presence of circumstellar material around main sequence stars, and looking for exocometary events. The work conc…

astro-ph.EP2017

DZ Cha: a bona fide photoevaporating disc

H. Canovas, B. Montesinos, M. R. Schreiber +14

DZ Cha is a weak-lined T Tauri star (WTTS) surrounded by a bright protoplanetary disc with evidence of inner disc clearing. Its narrow $\Ha$ line and infrared spectral energy distr…

astro-ph.EP2017

Evolution of protoplanetary disks from their taxonomy in scattered light: Group I vs. Group II

Antonio Garufi, Gwendolyn Meeus, Myriam Benisty +13

High-resolution imaging reveals a large morphological variety of protoplanetary disks. To date, no constraints on their global evolution have been found from this census. An evolut…

astro-ph.SR2016★ 35 cited

Exocomet signatures around the A-shell star Leo?

C. Eiroa, I. Rebollido, B. Montesinos +18

We present an intensive monitoring of high-resolution spectra of the Ca {\sc ii} K line in the A7IV shell star Leo at very short (minutes, hours), short (night to night), and m…

astro-ph.SR2016

Constraining the mass of the planet(s) sculpting a disk cavity. The intriguing case of 2MASS J16042165-2130284

H. Canovas, A. Hardy, A. Zurlo +10

The large cavities observed in the dust and gas distributions of transition disks may be explained by planet-disk interactions. At ~145 pc, 2MASS J16042165-2130284 (J1604) is a 5-1…