A HUBBLE SPACE TELESCOPE SURVEY OF H sub(2) EMISSION IN THE CIRCUMSTELLAR ENVIRONMENTS OF YOUNG STARS

• Published in: The Astrophysical journal 2012-09, Vol.756 (2), p.1-17
• Main Authors: France, Kevin, Schindhelm, Eric, Herczeg, Gregory J, Brown, Alexander, Abgrall, Herve, Alexander, Richard D, Bergin, Edwin A, Brown, Joanna M, Linsky, Jeffrey L, Roueff, Evelyne, Yang, Hao
• Format: Article
• Language: English
• Subjects: Accretion; Emission; Emittance; Formations; Hubble Space Telescope; Spatial distribution; Spectral lines; Spectrographs; T Tauri stars
• ISSN: 0004-637X; 1538-4357
• DOI: 10.1088/0004-637X/756/2/171

The formation timescale and final architecture of exoplanetary systems are closely related to the properties of the molecular disks from which they form. Observations of the spatial distribution and lifetime of the molecular gas at planet-forming radii (a < 10 AU) are important for understanding the formation and evolution of exoplanetary systems. Toward this end, we present the largest spectrally resolved survey of H sub(2) emission around low-mass pre-main-sequence stars compiled to date. We use a combination of new and archival far-ultraviolet spectra from the Cosmic Origins Spectrograph and Space Telescope Imaging Spectrograph instruments on the Hubble Space Telescope to sample 34 T Tauri stars (27 actively accreting Classical T Tauri Stars and 7 non-accreting Weak-lined T Tauri Stars) with ages ranging from ~1 to 10 Myr. We observe fluorescent H sub(2) emission, excited by Ly alpha photons, in 100% of the accreting sources, including all of the transitional disks in our sample (CS Cha, DM Tau, GM Aur, UX Tau A, LkCa 15, HD 135344B, and TW Hya). The spatial distribution of the emitting gas is inferred from spectrally resolved H sub(2) line profiles. Some of the emitting gas is produced in outflowing material, but the majority of H sub(2) emission appears to originate in a rotating disk. For the disk-dominated targets, the H sub(2) emission originates predominately at a [