58 citations · 333 across the 10 of their papers we have counts for
10 papers
Accretion signatures in the X-shooter spectrum of the substellar companion to SR12
Alejandro Santamaría-Miranda, Claudio Cáceres, Matthias R. Schreiber +5
About a dozen substellar companions orbiting young stellar objects or pre-main sequence stars at several hundred au have been identified in the last decade. These objects are inter…
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…
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…
The Detection of Dust around NN Ser
Adam Hardy, Matthias R. Schreiber, Steven G. Parsons +6
Eclipse timing variations observed from the post common-envelope binary (PCEB) NN Ser offer strong evidence in favour of circumbinary planets existing around PCEBs. If real, these…
Detached cataclysmic variables are crossing the orbital period gap
Monica Zorotovic, Matthias R. Schreiber, Steven G. Parsons +6
A central hypothesis in the theory of cataclysmic variable (CV) evolution is the need to explain the observed lack of accreting systems in the ~2-3 h orbital period range, known as…
A ring-like concentration of mm-sized particles in Sz 91
H. Canovas, C. Caceres, M. R. Schreiber +4
Models of planet formation and disc evolution predict a variety of observables in the dust structure of protoplanetary discs. Here we present Atacama Large Millimeter/submillimeter…
On the nature of the tertiary companion to FW Tau: ALMA CO observations and SED modeling
Claudio Caceres, Adam Hardy, Matthias R. Schreiber +7
It is thought that planetary mass companions may form through gravitational disk instabilities or core accretion. Identifying such objects in the process of formation would provide…
Probing the Final Stages of Protoplanetary Disk Evolution with ALMA
A. Hardy, C. Caceres, M. R. Schreiber +5
The evolution of a circumstellar disk from its gas-rich protoplanetary stage to its gas-poor debris stage is not understood well. It is apparent that disk clearing progresses from…
Gas inside the 97 au cavity around the transition disk Sz\,91
H. Canovas, M. R. Schreiber, C. Cáceres +9
We present ALMA (Cycle 0) band-6 and band-3 observations of the transition disk Sz\,91. The disk inclination and position angle are determined to be $i=49.5\degr\pm3.5\degr$ and $\…
The First Science Results from SPHERE: Disproving the Predicted Brown Dwarf around V471 Tau
A. Hardy, M. R. Schreiber, S. G. Parsons +10
Variations of eclipse arrival times have recently been detected in several post common envelope binaries consisting of a white dwarf and a main sequence companion star. The general…