Constraining the Evolution of Molecular Gas in Weak-Line T-Tauri Stars 1. Motivation The formation of planets from protoplanetary disks is greatly influenced by the presence or absence of gas in these disks. The mass an

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Date: 2009-09-08 18:47:50 Space Star types Protoplanetary disk Nebular hypothesis Debris disk T Tauri star T Tauri Star Photoevaporation Astronomy Stellar astronomy Star formation		Constraining the Evolution of Molecular Gas in Weak-Line T-Tauri Stars 1. Motivation The formation of planets from protoplanetary disks is greatly influenced by the presence or absence of gas in these disks. The mass an Add to Reading List Source URL: www.u.arizona.edu Download Document from Source Website File Size: 61,65 KB Share Document on Facebook

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