286 citations · 1.4k across the 35 of their papers we have counts for
7 papers · 1 filter
X-ray deficiency on strong accreting T Tauri stars - Comparing Orion with Taurus
Ignacio Bustamante, Bruno Merín, Hervé Bouy +3
Depending on whether a T Tauri star accretes material from its circumstellar disk or not, different X-ray emission properties can be found. The accretion shocks produce cool heatin…
Herschel-PACS observations of discs in the Eta Chamaeleontis association
P. Riviere-Marichalar, P. Elliott, I. Rebollido +6
Protoplanetary discs are the birthplace for planets. Studying protoplanetary discs is the key to constraining theories of planet formation. By observing dust and gas in association…
Infrared study of transitional disks in Ophiuchus with Herschel
Isabel Rebollido, Bruno Merín, Álvaro Ribas +7
Context. Observations of nearby star-forming regions with the Herschel Space Observatory complement our view of the protoplanetary disks in Ophiuchus with information about the out…
First detection of thermal radio jets in a sample of proto-brown dwarf candidates
O. Morata, A. Palau, R. F. González +10
We observed with the JVLA at 3.6 and 1.3 cm a sample of 11 proto-brown dwarf candidates in Taurus in a search for thermal radio jets driven by the most embedded brown dwarfs. We de…
Protoplanetary disk lifetimes vs stellar mass and possible implications for giant planet populations
Álvaro Ribas, Hervé Bouy, Bruno Merín
We study the dependence of protoplanetary disk evolution on stellar mass using a large sample of young stellar objects in nearby young star-forming regions. We update the protoplan…
Identification of new transitional disk candidates in Lupus with Herschel
I. Bustamante, B. Merín, Á. Ribas +4
New data from the Herschel Space Observatory are broadening our understanding of the physics and evolution of the outer regions of protoplanetary disks in star forming regions. In…
Messier 35 (NGC2168) DANCe I. Membership, proper motions and multi-wavelength photometry
H. Bouy, E. Bertin, D. Barrado +7
We aim at identifying the cluster's members by deriving membership probabilities for the sources within 1 degree of the cluster's center, going further away than equivalent previou…