181 citations · 544 across the 17 of their papers we have counts for
17 papers
Gravity or turbulence V: Star forming regions undergoing violent relaxation
Andrea Bonilla-Barroso, J. Ballesteros-Paredes, Jesus Hernández +6
Using numerical simulations of the formation and evolution of stellar clusters within molecular clouds, we show that the stars in clusters formed within collapsing molecular cloud…
A Core Mass Function Indistinguishable from the Salpeter Stellar Initial Mass Function Using 1000 au Resolution ALMA Observations
Genaro Suárez, Roberto Galván-Madrid, Luis Aguilar +4
We present the core mass function (CMF) of the massive star-forming clump G33.92+0.11 using 1.3 mm observations obtained with the Atacama Large Millimeter/submillimeter Array (ALMA…
Gaia kinematics reveal a complex lopsided and twisted Galactic disc warp
M. Romero-Gómez, C. Mateu, L. Aguilar +2
There are few warp kinematic models of the Galaxy able to characterise structure and kinematics. These models are necessary to study the lopsidedness of the warp and the twisting o…
Kinematic identification of young nearby moving groups from a sample of chromospherically active stars in the RAVE catalog
Valeria Ramírez-Preciado, Carlos G. Roman-Zuñiga, Luis Aguilar +2
The purpose of this study is the identification of young ( Myr), nearby ( pc) moving groups (YNMGs) through their kinematic signature. YNMGs could be…
Predictions for the detection of Tidal Streams with Gaia using Great Circle Methods
Cecilia Mateu, Andrew Cooper, Andreea S. Font +5
The Gaia astrometric mission may offer an unprecedented opportunity to discover new tidal streams in the Galactic halo. To test this, we apply nGC3, a great-circle-cell count metho…
An efficient positive potential-density pair expansion for modelling galaxies
Armando Rojas-Niño, Justin I. Read, Luis Aguilar +1
We present a novel positive potential-density pair expansion for modelling galaxies, based on the Miyamoto-Nagai (MN) disc. By using three sets of such discs, each one of them alig…