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Caustics of the restricted three-body problem
(Edp Sciences S A, 1998-03-01)
Trajectories of the planar, circular, restricted three-body problem are given in the configuration space through the caustics associated to the invariant tori of quasi-periodic orbits. It is shown that the caustics of ...
Caustics of the restricted three-body problem
(Edp Sciences S A, 1998-03-01)
Trajectories of the planar, circular, restricted three-body problem are given in the configuration space through the caustics associated to the invariant tori of quasi-periodic orbits. It is shown that the caustics of ...
Caustics of the restricted three-body problem
(1998-03-20)
Trajectories of the planar, circular, restricted three-body problem are given in the configuration space through the caustics associated to the invariant tori of quasi-periodic orbits. It is shown that the caustics of ...
Characterisation of young stellar clusters
(EDP SCIENCES S ALES ULIS CEDEX A, 2012)
Aims. Several embedded clusters are found in the Galaxy. Depending on the formation scenario, most of them can evolve to unbounded groups that are dissolved within 10 Myr to 20 Myr. A systematic study of young stellar ...
A Galactic ring of minimum stellar density near the solar orbit radius
(Oxford, 2014-04-10)
We analyse the secular effects of a long-lived Galactic spiral structure on the stellar orbits with mean radii close to the corotation resonance. By test-particle simulations and different spiral potential models with ...
Star Forming Regions Towards Stellar Wind Bubbles: RCW 52 and RCW 78
(2011)
We carried out observations of the continuum emission at 870 μm and the ^{13}CO(2-1) line towards star forming regions in the stellar wind bubbles RCW 52 and RCW 78 using the APEX telescope. The molecular observations ...
Stellar activity as a tracer of moving groups
(EDP Sciences, 2013)
We present the results of a study of the stellar activity in the solar neighborhood using complete kinematics (galactocentric velocities
U, V, W) and the chromospheric activity index log R0
HK. We analyzed the average ...
The molecular interstellar medium associated with the young compact stellar cluster Westerlund 1
(2011)
Analizamos el medio interestelar molecular en torno a Westerlund 1, el cúmulo estelar joven más masivo conocido en la Vía Láctea. Descubrimos una región molecular central evacuada entre dos complejos moleculares con ...
The molecular interstellar medium associated with the young compact stellar cluster Westerlund 1
(2011)
Analizamos el medio interestelar molecular en torno a Westerlund 1, el cúmulo estelar joven más masivo conocido en la Vía Láctea. Descubrimos una región molecular central evacuada entre dos complejos moleculares con ...