scispace - formally typeset
M

María José Maureira

Researcher at Max Planck Society

Publications -  26
Citations -  270

María José Maureira is an academic researcher from Max Planck Society. The author has contributed to research in topics: Protostar & Star formation. The author has an hindex of 9, co-authored 18 publications receiving 189 citations. Previous affiliations of María José Maureira include Yale University & University of Chile.

Papers
More filters
Journal ArticleDOI

Widespread Molecular Outflows in the Infrared Dark Cloud G28.37+0.07: Indications of Orthogonal Outflow-filament Alignment

TL;DR: In this paper, the position angle in the plane-of-sky of 120 CO outflow lobes and their distribution was determined from ALMA CO(2-1) observations toward a massive infrared dark cloud G28.37+0.07.
Journal ArticleDOI

Orbital and mass constraints of the young binary system IRAS 16293-2422 A

TL;DR: In this paper, the authors presented 3 mm ALMA continuum and line observations at resolutions of 6.5 au and 13 au, respectively, toward the Class 0 system IRAS 16293-2422 A. The ALMA high-resolution data provided a unique insight into the gas kinematics and masses of a young deeply embedded bound binary system.
Journal ArticleDOI

CASTING LIGHT ON THE ANOMALOUS STATISTICS OF Mg II ABSORBERS TOWARD GAMMA-RAY BURST AFTERGLOWS: THE INCIDENCE OF WEAK SYSTEMS

TL;DR: In this paper, the authors revisited the echelle spectra of eight gamma-ray burst (GRB) afterglows to obtain the incidence (dN/dz) of weak intervening Mgii systems at a mean redshift ofz �= 1.5.
Journal ArticleDOI

The Central 1000 au of a Prestellar Core Revealed with ALMA. II. Almost Complete Freeze-out

TL;DR: In this article , the first clear observational evidence of NH2D freeze-out toward the L1544 prestellar core was presented, indicating the presence of a complete depletion zone within a ≃1800 au radius.
Journal ArticleDOI

Kinematics of a young low-mass star-forming core: understanding the evolutionary state of the first-core candidate L1451-mm

TL;DR: In this article, the authors used 3mm multi-line and continuum CARMA observations towards the first hydrostatic core (FHSC) candidate L1451-mm to characterize the envelope kinematics at 1000 AU scales and investigate its evolutionary state.