The masses of young stars: CN as a probe of dynamical masses

2014/06/15 by S. Guilloteau, M. Simon, V. Piétu +4
Physics and Astronomy · #Astro and Planetary Science #Astrophysics and Star Formation Studies #Stellar, planetary, and galactic studies #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201423765

published as A&A 567, A117 (2014) · Astronomy & Astrophysics in press, 20 pages

arxiv created 2014/06/15 · openalex publication_date 2014/06/16 · arxiv updated 2014/09/05 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Aims. We attempt to determine the masses of single or multiple young T Tauri and HAeBe stars from the rotation of their Keplerian disks.

Citations

• Surprising dissimilarities in a newly formed pair of ‘identical twin’ stars
• Y 2 Isochrones with an Improved Core Overshoot Treatment
• The Dartmouth Stellar Evolution Database
• Disks around CQ Tauri and MWC 758: dense PDR or gas dispersal?
• Intrinsic Colors, Temperatures, and Bolometric Corrections of Pre-Main Sequence Stars