Consistent dust and gas models for protoplanetary disks. IV. A panchromatic view of protoplanetary disks
Constraints to the magnetospheric properties of T Tauri stars - II. The Mg II ultraviolet feature
Hot Gas Lines in T Tauri Stars
Multiepoch Ultraviolet HST Observations of Accreting Low-mass Stars
Panchromatic Imaging of a Transitional Disk: The Disk of GM Aur in Optical and FUV Scattered Light
Revealing the Star-Disk-Jet Connection in GM Aur Using Multiwavelength Variability
Structure and Dynamics of the Accretion Process and Wind in TW Hya
Twenty-five Years of Accretion onto the Classical T Tauri Star TW Hya
Using FUV to IR Variability to Probe the Star-Disk Connection in the Transitional Disk of GM Aur
Using Multiwavelength Variability to Explore the Connection among X-Ray Emission, the Far-ultraviolet H2 Bump, and Accretion in T Tauri Stars
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage
2010-01-28T23:11:40Z/2012-01-05T09:01:56Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Calvet comma Nuria, 2013, 'How Far Does H2 Go: Constraining FUV Variability in the Gaseous Inner Holes of Protoplanetary Disks', 1.0, European Space Agency, https://doi.org/10.5270/esa-troo3a5