Skip to content
Universidad del Mar SIBUMAR Descubridor Institucional UMAR
  • Inicio
  • Búsqueda avanzada
  • Explorar
  • Login
    • English
    • Deutsch
    • Español
    • Français
    • Italiano
Advanced
  • Differentiating Formation Models with New Dynamical Masses for the PDS 70 Protoplanets
Cover Image

Differentiating Formation Models with New Dynamical Masses for the PDS 70 Protoplanets

Fuente: arXiv
Saved in:
Bibliographic Details
Main Authors: Trevascus, David, Blunt, Sarah, Christiaens, Valentin, Matthews, Elisabeth, Hammond, Iain, Brandner, Wolfgang, Wang, Jason, Lacour, Sylvestre, Vigan, Arthur, Balmer, William O., Bonnefoy, Mickael, Burn, Remo, Chauvin, Gaël, Gratton, Raffaele, Houllé, Mathis, Hinkley, Sasha, Kammerer, Jens, Kreidberg, Laura, Marleau, Gabriel-Dominique, Mesa, Dino, Otten, Gilles, Nowak, Mathias, Rickman, Emily, Sanchez-Bermudez, Joel, Sauter, Jonas
Format: Preprint
Published: 2025
Subjects:
Earth and Planetary Astrophysics
Online Access:
Acceder al recurso
Tags: Add Tag
No Tags, Be the first to tag this record!
  • Cite this
  • Text this
  • Email this
  • Print
  • Export Record
    • Export to RefWorks
    • Export to EndNoteWeb
    • Export to EndNote
  • Save to List
  • Permanent link
  • Holdings
  • Description
  • Comments
  • Similar Items
  • Staff View

Internet

https://arxiv.org/abs/2504.11210

Similar Items

  • YSES 2b is a background star: Differential astrometric M-dwarf measurements in time
    by: Kenworthy, Matthew, et al.
    Published: (2025)
  • Evidence for Variable Accretion onto PDS 70 c and Implications for Protoplanet Detections
    by: Zhou, Yifan, et al.
    Published: (2025)
  • VLTI/GRAVITY Observations of AF Lep b: Preference for Circular Orbits, Cloudy Atmospheres, and a Moderately Enhanced Metallicity
    by: Balmer, William O., et al.
    Published: (2024)
  • Keplerian motion of a compact source orbiting the inner disc of PDS 70: a third protoplanet in resonance with b and c?
    by: Hammond, Iain, et al.
    Published: (2025)
  • SIMTERFERE: An optical interferometry simulator for quantifying the coherent flux stability of VLTI/GRAVITY+. Reaching per mill stability: Application to exoplanet spectroscopy
    by: Sauter, J. R., et al.
    Published: (2026)
Universidad del Mar
Universidad del MarSistema Bibliotecario de la Universidad del MarDescubridor Institucional UMARImplementación y desarrollo: Mtro. Carlos Alonso Albores Pérez
InicioBúsqueda avanzadaExplorar
Visitas al Descubridor: 33,245© 2026 Universidad del Mar