27 citations · 76 across the 7 of their papers we have counts for
9 papers
A train of shocks at 3000 au scale? Exploring the clash of an expanding bubble into the NGC 1333 IRAS 4 region. SOLIS XIV
Marta De Simone, Claudio Codella, Cecilia Ceccarelli +10
There is evidence that the star formation process is linked to the intricate net of filaments in molecular clouds, which may be also due to gas compression from external triggers.…
Two-wind interactions in binaries with two orbiting giant stars
A. Castellanos-Ramírez, A. Rodríguez-González, Z. Meliani +3
Some red giant envelopes present spiral structures (seen either in dust scattered stellar continuum or in molecular line emission), the most striking example probably being AFGL 30…
HCN/HNC chemistry in shocks: a study of L1157-B1 with ASAI
B. Lefloch, G. Busquet, S. Viti +9
HCN and its isomer HNC play an important role in molecular cloud chemistry and the formation of more complex molecules. We investigate here the impact of protostellar shocks on the…
An orbital release model for the Orion BN/KL fingers
A. C. Raga, P. R. Rivera-Ortiz, A. Rodriguez-Gonzalez +1
We present a simple model in which the bullets that produce the "Orion fingers" (ejected by the BN/KL object) are interpreted as protoplanets or low mass protostars in orbit around…
Explosive ejections generated by gravitational interactions
Pedro Ruben Rivera-Ortiz, Ary Rodríguez-González, Jorge Cantó +1
During the fragmentation and collapse of a molecular cloud, it is expected to have close encounters between (proto)stellar objects that can lead to the ejection of a fraction of th…
H mass-velocity relationship from 3D numerical simulations of jet-driven molecular outflows
Adriano Cerqueira, Bertrand Lefloch, Alejandro Esquivel +4
Previous numerical studies have shown that in protostellar outflows, the mass-velocity distribution can be well described by a broken power law . On the oth…