539 citations
- Ludwig-Maximilians-Universität MünchenDE139 papers
- Max Planck Institute for Extraterrestrial PhysicsDE79 papers
- Centre National de la Recherche ScientifiqueFR50 papers
- Max Planck Institute for AstrophysicsDE45 papers
- European Southern ObservatoryCL41 papers
- Max Planck Institute for AstronomyDE40 papers
- Instituto de Astrofísica de CanariasES38 papers
- Center for Astrophysics Harvard & SmithsonianUS34 papers
- Universidad de La LagunaES33 papers
- University of MichiganUS32 papers
- Leiden UniversityNL28 papers
- Institut d'Estudis Espacials de CatalunyaES27 papers
19 papers · 1 filter
FAUST XXX: Dust enhancement in the young binary L1551 IRS 5
Nicolás Cuello, Eleonora Bianchi, François Ménard +17
Young binary stars with discs provide unique laboratories to study the earliest stages of planet formation in star-forming environments. The detection of substructure in discs arou…
Probing accretion and stellar properties in the Orion Nebula with VLT/X-Shooter
L. Piscarreta, G. Beccari, R. A. B. Claes +6
Multiple photometric studies have reported the presence of seemingly older accreting pre-main sequence stars (PMS) in optical colour-magnitude diagrams (CMDs). We investigate this…
Detailed Microwave Continuum Spectra from Bright Protoplanetary Disks in Taurus
Caleb Painter, Sean M. Andrews, Claire J. Chandler +9
We present new observations that densely sample the microwave (4-360 GHz) continuum spectra from eight young systems in the Taurus region. Multi-component, empirical model prescrip…
Spatial distribution and clustering properties of the young stellar populations in the Carina Nebula complex and Car OB1
C. Göppl, T. Preibisch
We use Gaia DR3 astrometry and photometry to analyze the spatial distribution of the young stellar populations and stellar clusters and to search for new OB star candidates in the…
FAUST VIII. The protostellar disk of VLA 1623-2417 W and its streamers imaged by ALMA
S. Mercimek, L. Podio, C. Codella +25
More than 50% of solar-mass stars form in multiple systems. It is therefore crucial to investigate how multiplicity affects the star and planet formation processes at the protostel…
Empirical Determination of the Lithium 6707.856 Å Wavelength in Young Stars
Justyn Campbell-White, Carlo F. Manara, Aurora Sicilia-Aguilar +20
Absorption features in stellar atmospheres are often used to calibrate photocentric velocities for kinematic analysis of further spectral lines. The Li feature at 6708 Å is…