12 citations · 20 across the 4 of their papers we have counts for
5 papers
Filament Formation via Collision-induced Magnetic Reconnection -- Kinematic Features
Shuo Kong, Griselda Arroyo-Chávez, Volker Ossenkopf-Okada +4
The Collision-induced Magnetic Reconnection (CMR) mechanism has recently been proposed as a filament formation model that emphasizes the active role of magnetic fields. To enable b…
On the role of gravity, turbulence, and the magnetic field in angular momentum transfer within molecular clouds
Griselda Arroyo-Chavez, Enrique Vazquez-Semadeni, James Wurster
Observations of molecular structures on scales of pc show that the specific angular momentum () scales with radius () as . We study the effects o…
The Turbulent Support (TS) and Global Hierarchical Collapse (GHC) models for molecular clouds compared. Differences, convergence, and myths
Enrique Vázquez-Semadeni, Aina Palau, Gilberto C. Gómez +8
We provide a detailed comparison between the ``turbulent support'' (TS) and ``global hierarchical collapse'' (GHC) models for molecular clouds and star formation, their respective…
Evolution of the angular momentum during gravitational fragmentation of molecular clouds
G. Arroyo-Chávez, E. Vázquez-Semadeni
We investigate the origin of the observed scaling between the specific angular momentum and the radius of molecular clouds (MCs) and their their substructur…
Neutron and quark stars: constraining the parameters for simple EoS using the GW170817
Griselda Arroyo-Chávez, Alejandro Cruz-Osorio, F. D. Lora-Clavijo +2
It is well known that the equation of state (EoS) of compact objects like neutron and quark stars is not determined despite there are several sophisticated models to describe it. F…