681 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Centre National de la Recherche ScientifiqueFR190 papers
- Laboratoire d’Etudes du Rayonnement et de la Matière en Astrophysique et AtmosphèresFR83 papers
- Max Planck Institute for AstronomyDE82 papers
- Sorbonne UniversitéFR77 papers
- Université Paris Sciences et LettresFR75 papers
- National Radio Astronomy ObservatoryUS74 papers
- Laboratoire d'Astrophysique de BordeauxFR65 papers
- Université de BordeauxFR63 papers
- Institut de Recherche en Astrophysique et PlanétologieFR59 papers
- Center for Astrophysics Harvard & SmithsonianUS58 papers
- Max Planck Institute for Radio AstronomyDE53 papers
- Université Grenoble AlpesFR53 papers
5 papers · 2 filters
On the central symmetry of the circumstellar envelope of RS Cnc
Pham Tuyet Nhung, Do Thi Hoai, Jan Martin Winters +3
We present a phenomenological study of CO(1-0) and CO(2-1) emission from the circumstellar envelope (CSE) of the Asymptotic Giant Branch (AGB) star RS\,Cnc. It reveals departures f…
The ALMA view of the protostellar system HH212 - The wind, the cavity, and the disk
C. Codella, S. Cabrit, F. Gueth +8
Context: Because it is viewed simply edge-on, the HH212 protostellar system is an ideal laboratory for studying the interplay of infall, outflow, and rotation in the earliest stage…
The masses of young stars: CN as a probe of dynamical masses
S. Guilloteau, M. Simon, V. Piétu +4
Aims: We attempt to determine the masses of single or multiple young T Tauri and HAeBe stars from the rotation of their Keplerian disks. Methods:We used the IRAM PdBI interferomete…
GG Tau: the fifth element
E. Di Folco, A. Dutrey, J. -B. Le Bouquin +9
We aim at unveiling the observational imprint of physical mechanisms that govern planetary formation in young, multiple systems. In particular, we investigate the impact of tidal t…
The multi-scale environment of RS Cnc from CO and HI observations
D. T. Hoai, L. D. Matthews, J. M. Winters +4
We present a detailed study of the circumstellar gas distribution and kinematics of the semi-regular variable star RS Cnc on spatial scales ranging from ~1" (~150 AU) to ~6' (~0.25…